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1 FREQUENCY DIVISION MULTIPLE ACCESS RECEIVER FOR WIRELESS INTERCONNECTION ON PRINTED CIRCUIT BOARDS By MINSOON HWANG A DISSERTATION PRESENTED TO THE GRADUATE SCHOOL OF THE UNIVERSITY OF FLORIDA IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY UNIVERSITY OF FLORIDA 2011

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FREQUENCY DIVISION MULTIPLE ACCESS RECEIVER FOR WIRELESS INTERCONNECTION ON PRINTED CIRCUIT BOARDS

By

MINSOON HWANG

A DISSERTATION PRESENTED TO THE GRADUATE SCHOOL OF THE UNIVERSITY OF FLORIDA IN PARTIAL FULFILLMENT

OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY

UNIVERSITY OF FLORIDA

2011

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© 2011 Minsoon Hwang

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To my wife, son, daughter and parents

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ACKNOWLEDGMENTS

I want to express my deep gratitude and appreciation to my advisor, Professor

Kenneth K. O, for his patient, constant encouragement and devotion. He guided me

through the transition from a student to an electrical engineer. Under his supervision, I

had opportunities to work in microelectronics, which eventually became a joy for me.

Also much appreciation goes to Professor William Eisenstadt, Huikai Xie and Professor

Namho Kim for their helpful suggestions to my research. I would like to thank them for

their interests in this work and serving on my Ph.D. supervisory committee

Much appreciation goes to TOYOTA Motor Corporation for funding this work and

Dr. Janshen Lin and Dr. Rizwan Bashillulah to help me with measurement equipment. I

also would like to thank the SiMICS members Yu Su, Yanping Ding, Eunyoung Seok,

Swaminathan Sankaran, Kwangchun Jung, Chikuang Yu, Haifeng Xu, Jau-Jr Lin, Ning

Zhang, Hisnta Wu, Chuying Mao, Dongha shim, Tie Sun, Hsinta Wu, Dongha Shim, Tie

Sun, Wuttichai Lerdsitomboon, Ruonan Han, Dr. Choongyul cha, and Kyungsun Seol. It

was quite fortunate to have worked with my colleagues. The discussions with them and

their advice were immensely helpful for completing this work. Finally, I deeply thank to

my wife, son, daughter and parents for their love and support through the lengthy Ph.D.

program.

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TABLE OF CONTENTS page

ACKNOWLEDGMENTS .................................................................................................. 4

LIST OF TABLES ............................................................................................................ 7

LIST OF FIGURES .......................................................................................................... 8

LIST OF ABBREVIATIONS ........................................................................................... 14

ABSTRACT ................................................................................................................... 16

CHAPTER

1 INTRODUCTION .................................................................................................... 18

1.1 Hybrid Circuit Board Using Photo Couplers ...................................................... 18 1.2 How to Improve Hybrid Engine Controller Board .............................................. 19 1.3 Organization of the Dissertation ........................................................................ 22

2 SYSTEM OVERVIEW ............................................................................................. 23

2.1 Hybrid Engine Controller Communication System ............................................ 23 2.2 FDMA Channel Link Analysis ........................................................................... 25 2.3 FDMA Receiver Architecture ............................................................................ 26

3 RF TO IF CONVERSION OF FDMA RECEIVER ................................................... 29

3.1 On-Chip Antenna and Duplexer ........................................................................ 29 3.1.1 Overview of On-Chip Antenna ................................................................. 29 3.1.2 Duplexer .................................................................................................. 34

3.2 Broadband Low Noise Amplifier ........................................................................ 36 3.4 Band Pass Filter ............................................................................................... 51 3.4 Broadband RF Amplifier .................................................................................... 54 3.5 Broadband Down Conversion Mixer ................................................................. 57

4 INTERMEDIATE FREQUENCY TO BASEBAND CONVERSION .......................... 68

4.1 IF-to Baseband Conversion System ................................................................. 68 4.1.1 Intermediate Frequency Amplifier ............................................................ 69 4.1.2 IF to BB Down Conversion Mixer ............................................................ 73

4.2 Baseband Architecture ...................................................................................... 80 4.3 Measurement Results ....................................................................................... 84

5 SYNTHESES OF MULTIPLE INTERMEDIATE FREQUENCIES ........................... 89

5.1 Background of Frequency Generation .............................................................. 89

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5.2 Frequency Generation and Duty Correction ..................................................... 91 5.3 Phase Generation ............................................................................................. 97 5.4 Measurement of Test Structure ...................................................................... 100 Summary .............................................................................................................. 112

6 FDMA RECEIVER CHARACTERIZATION ........................................................... 114

6.1 Test Structure ................................................................................................. 114 6.2 Measurements of FDMA Receiver Chain ........................................................ 117

6.2.1 RF Front-End Measurements ................................................................ 117 6.2.2 RF-to-Baseband Converter measurements ........................................... 119

6.2 Time Shared FDMA Receiver ......................................................................... 126

7 SUMMARY AND SUGGESTED FUTURE WORKS ............................................. 132

7.1 Summary ........................................................................................................ 132 7.2 Suggested Future Work .................................................................................. 133

LIST OF REFERENCES ............................................................................................. 134

BIOGRAPHICAL SKETCH .......................................................................................... 140

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LIST OF TABLES

Table page 2-1 Frequency plan for Channels of CDMA and FDMA link ( unit : GHz) ................. 24

2-2 Link margin analysis for the FDMA channel link ................................................. 26

3-1 Specification of the on-chip duplexer [28] ........................................................... 35

3-2 Bandwidth versus n [42] ..................................................................................... 39

3-3 Performance of LNAs over 20 GHz .................................................................... 50

5-1 Intermediate frequency and frequency divider ratio ............................................ 89

5-2 Phases difference generated by IF generator according to frequencies ............. 98

5-3 Frequency and phase selection ........................................................................ 100

5-4 Summary of IF generator measurement ........................................................... 112

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LIST OF FIGURES

Figure page 1-1 Hybrid cars selling in North America [1] – [7] ...................................................... 18

1-2 Hybrid engine controller board............................................................................ 19

1-3 Two approaches to replace photo-couplers ........................................................ 20

1-4 Communication system architecture of the hybrid engine controller board ........ 21

2-1 Block diagram of transceiver for the controller section with an FDMA transmitter and a CDMA receiver. ...................................................................... 24

2-2 Block diagram of transceiver architecture for the Deadtime controller with a CDMA transmitter and an FDMA receiver .......................................................... 25

2-3 The Proposed architecture of FDMA receiver..................................................... 27

2-4 Frequency plan for down conversion scheme of FDMA receiver ........................ 28

3-1 On-chip antenna A) Die photo of an on-chip antenna fabricated using UMC 130nm CMOS technology B) Cross section of an on-chip antenna.. .................. 29

3-2 3-mm zigzag antenna radiation pattern at 24 GHz [22] ...................................... 30

3-3 Antenna pair gain versus distance in the lobby of new engineering Building at 24 GHz. .............................................................................................................. 31

3-4 Measurement points chosen on the PCB [28] .................................................... 32

3-5 Large scale fading channel measurement results. ............................................. 33

3-7 Schematic of the single-ended on-chip duplexer [29] ......................................... 35

3-8 Die photo of the single-ended on-chip duplexer. ................................................ 36

3-9 Schematics of broadband LNA. .......................................................................... 37

3-10 Schematic of 5-stages gain distributed broadband differential LNA. .................. 40

3-11 Simple diagram and equivalent circuit of common source (CS) LNA A) Simple CS LNA schematic B) Equivalent circuit of CS LNA ............................... 40

3-12 Noise model of CS LNA ...................................................................................... 42

3-13 Schematic of differential common source (CS) amplifier with source degeneration inductor. ........................................................................................ 43

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3-14 Simulation results of differential common source (CS) LNA. Overall gain and gain of each stage versus frequency .................................................................. 44

3-15 The S-parameter and noise figure simulation results of differential common source (CS) LNA. ............................................................................................... 44

3-16 Measurement setup for 5 stage gain distributed differential LNA ....................... 45

3-17 Characterization set up for Balun plus GSSG probe using a network analyzer.[46]. ...................................................................................................... 45

3-18 Measurement setup for single ended mode. ...................................................... 46

3-19 Simulated S parameters and Noise Figure in single ended mode and differential mode A) S11 B) S21 C) S22 D) Noise Figure ................................... 47

3-20 Measured S-parameters in single ended mode. ................................................. 48

3-21 Deembeded |S21| and noise figure of LNA A) |S21| B) noise figure ..................... 48

3-22 Linearity measurement result of LNA A) IP1dB B) IIP3 ......................................... 49

3-23 Die photo of common source (CS) LNA. ............................................................ 51

3-24 Frequency plan of RF to IF conversion ............................................................... 51

3-25 Schematic of 3rd order Chevyshev band pass filter (BPF). ................................. 52

3-26 S-parameter simulation results versus frequency of 3rd order Chevyshev band pass filter (BPF) ......................................................................................... 52

3-27 Simulated phase versus frequency of 3rd order Chevyshev band pass filter (BPF) with ideal LC components and LC components including parasitics. ....... 53

3-28 Die photograph of 3rd order Chevyshev band pass filter (BPF) .......................... 53

3-29 Schematic of a 3-stages gain distributed cascode RF amplifier (RFA). .............. 54

3-30 S parameter measurement results of a 3-stages gain distributed cascode RFA and a bandpass filter in single ended mode. .............................................. 54

3-31 Measured |S21| in single ended mode and deembeded one in differential mode of a bandpass filter and a RFA. ................................................................ 55

3-32 Measured noise Figure in single ended mode and deembeded one in differential mode of a bandpass filter and a RFA ................................................ 55

3-33 Linearity measurement results of bandpass filter (BPF) and RFA combination A) IP1dB B) IIP3 ..................................................................................................... 56

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3-35 Single-balanced mixer A) schematic B) functional representation for the large switching signals ................................................................................................. 58

3-36 Double balanced Gilbert cell mixer ..................................................................... 59

3-37 Frequency translation of white noise in transconductor stage. ........................... 61

3-38 Time varying transconductance of the switching pair and the PSD of generated thermal noise [52] .............................................................................. 63

3-39 Schematic of double balanced Gilbert cell mixer with source degeneration inductors ............................................................................................................. 64

3-40 Voltage gain versus intermediate frequency (IF) as function of load resistance. .......................................................................................................... 65

3-41 Voltage gain and power gain versus input power. .............................................. 66

3-42 Noise figure versus intermediate frequency (IF) as function of load resistance .. 66

3-43 Die photograph and layout of broadband double balanced Gilbert cell mixer A) Die photograph B) Layout. ............................................................................. 67

4-1 Block diagram for IF to baseband conversion..................................................... 68

4-2 Schematic of broadband IF amplifier with resistive feedback ............................. 70

4-3 Schematic of single stage of resistive feedback inverter and equivalent circuit.. ................................................................................................................ 70

4-4 Layout of a differential IF amplifier with resistive feedback ................................. 72

4-5 Frequency plan of IF to BB conversion ............................................................... 73

4-6 Zero IF down conversion scheme using simple homodyne architecture ............ 74

4-8 Square wave with 50% duty cycle ...................................................................... 76

4-9 Power spectral density (PSD) of square wave with 50 % duty cycle. ................. 78

4-10 Schematic of double balanced Gilbert cell mixer ................................................ 79

4-11 Layout of double balanced Gilbert cell mixer. ..................................................... 80

4-12 Block diagram of baseband section of the FDAM receiver ................................. 81

4-13 Schematic of the third order low pass filter ......................................................... 81

4-14 Layout of the third order low pass filter ............................................................... 82

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4-15 Schematic of 3-stage baseband amplifier ........................................................... 82

4-16 Layout of the baseband amplifier ........................................................................ 83

4-17 Schematic of comparator and SR latch .............................................................. 83

4-18 Layout of comparator and SR latch .................................................................... 84

4-19 Measurement setup and test structure of the mixer and baseband amplifier integrated with an FDMA receiver. ..................................................................... 85

4-20 Input measurement scheme of IF to BB converter test structure ........................ 85

4-21 Measurement setup and PCB board of IF to BB converter test structure ........... 86

4-22 Measurement results of IF to baseband conversion stage ................................. 86

4-23 Measurement results of LPF and baseband amplifier A) Frequency response at baseband B) Gain of the LPF and BB amplifier .............................................. 87

5-1 Simplified frequency generation scheme ............................................................ 90

5-2 Generation of 2.8 GHz using a mixer and a high pass filter (HPF) ..................... 91

5-3. Schematic of current mode logic (CML) static divide-by-2 based on a D flip-flop [70] A) Block diagram of divide-by-2 circuit B) Schematic............................ 92

5-4 Block diagram and waveforms of a divide-by-2.5 ............................................... 93

5-5 Duty cycle correction scheme for the divide-by-2.5 and waveform to generate 2.4 GHz output. .................................................................................................. 93

5-6 Block diagram and waveforms of a divide-by-1.5 circuit. .................................... 94

5-7 Duty correction scheme for the divide-by-1.5 and waveforms. ........................... 95

5-9 Block diagram and waveforms of a divide-by-3 circuit using three dual edge triggered flip-flops (DEDFFs) .............................................................................. 97

5-10 Waveforms of a divide- by-2 circuit. .................................................................... 98

5-11 Waveforms of a divide-by-2.5 ............................................................................. 99

5-12 Waveforms of a divide-by-3 ................................................................................ 99

5-13 Measurement scheme and Die photograph of IF generator A) Measurement scheme and layout B) Die photograph ............................................................. 101

5-14 Printed Circuit Board (PCB) of IF generator testing. ......................................... 102

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5-15 Measurement setup for IF generator testing ..................................................... 102

5-16 Output spectra of IF generator A) 400 MHz B) 800 MHz C) 1.2 GHz D) 1.5 GHz E) 2.0 GHz F) 2.4 GHz G) 3.0 GHz .......................................................... 103

5-17 Measured duty cycle ratio of output waveforms of IF generator in the Oscilloscope Agilent® infiniium 86100B ........................................................... 105

5-18 Measured output waveforms of 400 MHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH. ............................................................... 107

5-19 Measured output waveforms of 800 MHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH. ............................................................... 108

5-20 Measured output waveforms of 1.2 GHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH. ............................................................... 108

5-21 Measured output waveforms of 1.5 GHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH. ............................................................... 109

5-22 Measured output waveforms of 2.0 GHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH. ............................................................... 109

5-23 Measured output waveforms of 2.4 GHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH. ............................................................... 110

5-24 Measured output waveforms of 3.0 GHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH. ............................................................... 110

5-24 Measured Phase Noise of each channel and input reference signal. ............... 111

6-1 Test structure of FDMA receiver. ...................................................................... 114

6-2 Test scheme and measurement setup of FDMA receiver ................................. 115

6-3 Die photo of transceiver at Deadtime controller ................................................ 116

6-4 Measurement scheme for RF Front-End of FDMA receiver ............................. 117

6-5 Measurement results of Duplexer for Antenna and FDMA receiver ports [72]. . 118

6-6 Gain of RF-Front-End of FDMA receiver .......................................................... 118

6-7 Measurement setup of IF to BB Down conversion ............................................ 119

6-8 Measured output power of IF-to-BB Mixer and Baseband amplifier (BBA) with -50 dBm RF input power for each channels ..................................................... 120

6-9 Gain of LNA to Baseband amplifier of FDMA receiver. ..................................... 122

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6-10 Measurement setup for ASK modulated data of FDMA receiver ...................... 122

6-11 Spectrum of ASK modulated PRBS data ......................................................... 123

6-12 Output waveforms of IF-to BB Mixer and ones of Inverted input data with 50 Mbps data rate A) 1110 1100 Pattern B) PRBS data ....................................... 124

6-13 Output waveforms of FDMA receiver and ones of Inverted input data with 50 Mbps data rate A) 111110000 B) 1110011000 ................................................ 124

6-14 Noise Figure measurement result of FDMA receiver ........................................ 125

6-15 Linearity measurement result of FDMA receiver A) IP1dB B) IIP3. ..................... 125

6-16 Block diagram of time shared FDMA receiver architecture. .............................. 127

6-17 Channel selection scheme of time shared FDMA receiver ............................... 127

6-18 Block diagram of 1-to-7 serial to parallel converter ........................................... 128

6-19 Test plan with two PCB board for the time shared FDMA receiver. .................. 129

6-20 Test structure of time shared FDMA receiver for three channels ...................... 129

6-21 Waveforms of test structure of time shared FDMA receiver for two channels .. 130

6-22 Output and selector waveforms of test structure of time shared FDMA receiver for two channels A) IF-to BB Mixer output B) Buffer output. ............... 131

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LIST OF ABBREVIATIONS

BB Baseband

BPF Band Pass Filter

C Capacitor

CDMA Code Division Multiple Access

CMOS Complementary Metal Oxide Semiconductor

CS Common source

FDMA Frequency Division Multiple Access

HPF High Pass Filter

GSSG Ground-Signal-Signal-Ground

IF Intermediate Frequency

IIP3 Input Third Order Intermodulation Intercept Point

IP1dB 1dB Input Compression Point

L Inductor

LC Inductor-Capacitor

LPF Inductor-Capacitor

LNA Low Pass Filter

NF Noise Figure

PCB Printed Circuit Board

Q Quality Factor

R Resistor

RC Resistor-Capacitor

RF Radio Frequency

RFA Radio Frequency Amplifier

SR Latch Set-Reset Latch

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RX Receiver

TX Transmitter

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Abstract of Dissertation Presented to the Graduate School of the University of Florida in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy

FREQUENCY DIVISION MULTIPLE ACCESS RECEIVER FOR WIRELESS

INTERCONNECTION ON PRINTED CIRCUIT BOARDS

By

Minsoon Hwang

August 2011

Chair: Kenneth K. O Major: Electrical and Computer Engineering

The return voltage levels of high voltage motor drive sections and a low voltage

digital control section in an engine controller board of a Hybrid Electric Vehicles (HEV)

can differ by several hundreds of volts. Presently, the board utilizes numerous photo-

couplers that can support ~1 Mbps data rate. Use of wireless inter-chip data

communication utilizing single chip radio integrating on-chip antennas to isolate return

paths is proposed. In particular, for communication from high voltage section to the low

voltage section, FDMA is selected to support seven data channels.

An FMDA receiver that can support seven 400-MHz channels form 24.2 to 27.2

GHz is implemented in the UMC 130 nm logic CMOS process. There are two major

parts in the FDMA receiver: receiver and local oscillator generation blocks.

A five stage gain distributed LNA, a BPF and three stage distributed RFA have

been demonstrated. The LNA has 19-dB gain and 5.7-dB noise figure at 30 GHz

consuming 49.5-mW power. The BPF and RFA combination has 5.2-dB gain and 11.4-

dB noise figure at 30 GHz.

The IF LO generator has been demonstrated. It utilizes only dividers composed of

DFF and buffers, and does not require a mixer or a filter. Dividers are shared and the

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total numbers of dividers in is only nine. To reduce the even harmonic effect, every LO

outputs have 50% duty cycle and their deviation is less that ±5% in single ended

measurements and ±1% in differential measurements. Each LO signal has two

selectable phases with difference greater than 60o. The phase offsets from the targets

are less than 8%.

A full FDMA receiver test structure has been demonstrated for seven channels.

The channels were characterized one at a time using a multiplexer that selects the IF

LO frequency. The gain of receiver from LNA to Baseband amplifier is 40 dB and noise

figure is 8.7 dB at 27 GHz at 242.3-mW power consumption.

Time shared FDMA receiver operation has been demonstrated up to data rate of

10 Mbps. Two channels are time shared using selection signal. It multiplexes two LO

signals with different frequencies.

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CHAPTER 1

INTRODUCTION

1.1 Hybrid Circuit Board Using Photo Couplers

Recently Hybrid electric Vehicles (HEV’s) have become popular item in the

automobile industry with the increasing gasoline price and the enactment of regulations

for carbon dioxide emissions in some countries. Because HEV’s have ~ 50% higher

gasoline mileage comparing with the same size vehicles with a gasoline only engine,

HEV’s can reduce the amount of carbon dioxide emission. HEV’s have been called

environment-friendly or eco-friendly cars. Many automobile makers have been

developing hybrid electric vehicles shown in Figure 1.1.

Figure 1-1. Hybrid cars selling in North America [1] - [7]

One of drawbacks of the HEV’s is high price. Lowering manufacturing cost has

been the main issue to make them widely accepted and utilized. There are so many

parts in an automobile. One of them is the hybrid engine controller board which checks

the statues and controls the operation of engine.

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Figure 1-2. Hybrid engine controller board

A hybrid engine controller board is shown in Figure1.2. This has photo-couplers to

communicate between the high voltage motor drive and low voltage control sections.

This research focuses on lowering the cost and improving the performance of hybrid

engine controller board by finding a new cheaper and better way to communicate

between sections. This proposed research investigates an approach using

complementary metal oxide semiconductor (CMOS) technology that reduces the

number of components for inter-chip communication and cost.

1.2 How to Improve Hybrid Engine Controller Board

The reason to use photo-couplers in the hybrid engine controller board shown in

Figure 1-2 is due to the potential difference in the signal return paths. This board is

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divided into two sections. One is the motor driver section that operates in high voltage.

The potential difference between the return paths can be as high as 300V. The other is

control section that operates at lows between 3 to 12 V. Photo-couplers, however, have

normally low transmission data rate of ~ 1 Mbits/sec. and costs ~ $1. For higher data

rate, they can cost up to many dollars.

RXTX

0 V

1.2 V

300 V

301.2 V

Single chip

A

Wireless

MotorController

PLL

TX

RX TX

RX

Deadtimecontroller

PLL

B Figure 1-3. Two approaches to replace photo-couplers A) Inductive coupling with

transformer in a single chip B) Wireless interconnection with on-chip antenna

Two approaches to replace photo couplers in the board have proposed [8]. The

left diagram in Figure 1-3 is an isolator that uses inductive coupling with a transformer.

The right one is a transceiver with on- chip antennas. The first approach was

investigated by Hsinta Wu using UMC 0.13 µm standard CMOS technology. The

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isolator could support 160 Mbits/sec. data rate at 70 V. The result was not sufficient to

support the 300-V difference due to the break down voltage limitation. For the second

approach, the feasibility of using on-chip antennas for wireless communications have

been studied [9]-[12] and integrated with other circuit blocks. Communication using on-

chip antenna is possible at 5 GHz and higher [13] [14]. There are 26 photo couplers in

the hybrid engine controller board. The focus of this proposed research is to optimize

transceivers with an on-chip antenna that can be used for communication from the high

voltage section to low voltage section.

Figure 1-4. Communication system architecture of the hybrid engine controller board

The communication system architecture of the hybrid engine board is shown in

Figure 1-4 [15]. This block diagram describe a half of the full system. There are 13

channels. This system consists of a Deadtime controller in the control section and 6

drivers and a temperature sensor in the motor section. Two different multiple access

methods are adapted for this system. The uplink uses frequency division multiple

access (FDMA), while the downlink uses code division multiple access (CDMA). The

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proposed research focuses on the receiver part of FDMA link and seeks that works with

the transmitter demonstrated by Hsinta Wu [15].

1.3 Organization of the Dissertation

First, the system and FDMA link will be discussed and the FDMA receiver

architecture are proposed in Chapter 2. In Chapter 3, radio frequency (RF) to

intermediate frequency (IF) conversion scheme are presented. Components

compromising the RF-font-end such as on-chip antenna, duplexer, broadband low noise

amplifier (LNA), band pass filter, RF amplifier, and broadband double balanced down

conversion mixer are discussed. In Chapter 4, IF to baseband conversion stage is

introduced, and IF amplifier and IF to baseband mixer are discussed. In Chapter 5, the

synthesis of local oscillator signals at multiple intermediate frequencies is discussed.

Generating seven different frequencies with two phases using simple and small circuits

such as dividers composed of D flip-flops is discussed. In Chapter 6, the baseband

architecture including components such as 3rd order low pass filter (LPF), baseband

amplifier, comparator and latch is discussed. In Chapter 7, measurement results of

FDMA receiver are presented. A time shared architecture for the FDMA receiver are

discussed and preliminary operation is demonstrated in Chapter 9. Lastly in Chapter 10,

the dissertation is summarized and future works are suggested

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CHAPTER 2 SYSTEM OVERVIEW

2.1 Hybrid Engine Controller Communication System

In the wireless interconnection system, there are two links, CDMA for down link,

FDAM for uplink [16]. Channelization is needed for the communication system to

support multiple channels. First looking at the requirement of CMDA link, the data rate

of each channel is 50 Mbps. The Walsh code is widely used for CDMA system. It has N

orthogonal codes per N bits (N is 1, 2, 4 , 8, … , 2N). Because there are six channels in

the CDMA link, 8 Walsh codes are required and chip rate is 400 Mcps (Mega chips per

second) or 8 times the data rate. A square wave has ~ 80% of the signal energy within

the first 3 harmonics. To capture these, the baseband bandwidth for CDMA links was

set to three times the chip rate, The RF bandwidth of CDMA link is 2.4 GHz which is

twice the bandwidth at baseband for an AM system [17]. The CDMA down link for six

channels are allocated at 16.8 GHz with a single carrier and data are spread from 15.6

to 18 GHz as shown in Table 2-1.

The FDMA link, on the other hand, has seven channels with 50 Mbps data rate for

each. A channel of FDAM link occupies 300 MHz bandwidth. The seven channels are

allocated at 24.4, 24.8, 25.2, 25.5, 26.0, 26.4, and 30.0 GHz. To support the multiple

access schemes, an FDMA receiver and a CDMA transmitter are needed for the

Deadtime controller in the control section. In the motor section, an FDMA transmitter

and a CDMA receiver are needed. A block diagram of transceiver for the motor section

is shown in Figure 2-1[18]. This is composed of an FDMA transmitter, a CDMA receiver,

PLL and clock data recovery (CDR) for LO frequency generation and data recovery, and

a 3-bit analog to digital converter.

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Table 2-1. Frequency plan for Channels of CDMA and FDMA link ( unit : GHz) TX Channel Freq. Band RX Channel Freq. Band Chip

Motor Controller 1 24.2-24.6 1 15.6-18, C1 M1 2 24.6-25.0 2 15.6-18, C2 M2 3 25.0-25.35 3 15.6-18, C3 M3 4 25.35-25.7 4 15.6-18, C4 M4 5 25.8-26.2 5 15.6-18, C5 M5 6 26.2-26.6 6 15.6-18, C6 M6 7 26.6-27.0 - - M7

Deadtime Controller 1 15.6-18, C1 1 24.2-24.6

D1

2 15.6-18, C2 2 24.6-25.0 3 15.6-18, C3 3 25.0-25.4 4 15.6-18, C4 4 25.4-25.8 5 15.6-18, C5 5 25.8-26.2 6 15.6-18, C6 6 26.2-26.6 - 7 26.6-27.0

Figure 2-1. Block diagram of transceiver for the controller section with an FDMA transmitter and a CDMA receiver

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The proposed architecture of other transceiver for the Deadtime controller side is

shown in Figure 2-2. There are two sections; a CDMA transmitter and an FDMA

receiver. The Deadtime controller sends signals to six CDMA receivers in Figure 1-4

through a duplexer and an on-chip antenna sharing with the FDMA receiver. The latter

has wider bandwidth than its counterpart transmitter because of the guard bands. Each

components of the FDMA receiver must support 3 GHz bandwidth.

Figure 2-2. Block diagram of transceiver architecture for the Deadtime controller with a CDMA transmitter and an FDMA receiver

2.2 FDMA Channel Link Analysis

The FDMA link in the hybrid engine controller board must support data rate of 50

Mbps/channel, latency less than 2 µs and a range of up to 15 cm. The board size is 15

cm x 25 cm. The link margin analysis of FDMA channel is shown in Table 2-2. The

maximum distance between chips is 15 cm and Eb/No is 14.5 dB for Amplitude shift

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keying (ASK) modulation to achieve 1X10-13 BER [19]. The sensitivity of this link is -74.3

dBm when the noise figure of a receiver is assumed 8 dB. Assuming that an on-chip

antenna on a 100-μm thick substrate has a -7 dB of antenna gain, the received power is

-57 dBm when the output power level of a transmitter is 3 dBm and propagation loss is

46 dB at the highest possible frequency of 32 GHz for the proposed system. The link

margin of FDMA channel, therefore, is 17.3 dB.

Table 2-2. Link margin analysis for the FDMA channel link FDMA link

Range (R) 15 cm TX Power 3 dBm Propagation Loss @ 32 GHz (λ/4πR) 2 46dB Antenna Gain (0.25λ = 3.2 mm) - 7 dB Received power -57 dBm

Thermal Noise [kT (oK)] -173.8 dBm/Hz Bandwidth (50 MHz) 77 dB Eb/No for BER of 1x10-13 for ASK 14.5 dB RX noise figure 8 dB Sensitivity -74.3 dBm Link margin 17.3 dB

2.3 FDMA Receiver Architecture

From the link margin analysis and system requirements for the hybrid engine

controller board, the architecture and design targets of FDMA receiver are specified in

this chapter. Considering the composition and frequency plan of Deadtime controller, a

duplexer is needed to isolate FDMA signals at 24.2 to 27.2 GHz from the CDMA ones at

15.6 to 18GHz. Another key to replace the photo couplers is an on-chip antenna

integrated with other circuitries There are seven channels from 24.2 through 27.2 GHz.

Seven receivers are required to down-convert seven different channels at the same

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time. This scheme, however, need more space and power. Simplification is needed to

lower cost. For instant, the RF front-end components such as a low noise amplifier

(LNA), a band pass filter (BPF), an RF to IF down-conversion mixer, and IF amplifier

(IFA) can be shared. The proposed architecture of FDMA receiver is shown in Figure 2-

3. This can be divided into two parts. One is part which converts RF signals coming

through an on-chip antenna to baseband signals.

Figure 2-3. The Proposed architecture of FDMA receiver

The other is a signal generation block with a phase locked loop (PLL) to generate

the necessary local oscillator frequencies for the RF to IF down conversion mixer and

an IF local oscillator (LO) frequency generator for IF to baseband down conversion

mixers. The RF and IF components in the proposed architecture, an LNA, a BPF, a

mixer, and an IF amplifier, have broad bandwidth to support the FDMA channels with 3

GHz bandwidth. The number of IF to baseband converters is seven. In the IF stage, the

signal of seven channels are allocated at 0.4, 0.8, 1.2, 1.5, 2.0, 2.4, and 3.0 GHz. This

means each channel needs different LO frequency for data recovery at the baseband.

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Figure 2-4 shows how each channel is converted down to baseband. First, RF signal is

translated to IF using the 24 GHz signal from the PLL. IF signals, then, are converted to

baseband using matched IF frequency LO signal. The baseband signals of seven

channels are filtered by a low pass filter, amplified, and converted to digital signals by a

comparator. For this system, a problem is simultaneously generating the seven different

LO signals. A goal of this proposed research is simplifying the architectures. This will be

explained in greater detail in Chapter 5.

Figure 2-4. Frequency plan for down conversion scheme of FDMA receiver

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CHAPTER 3 RF TO IF CONVERSION OF FDMA RECEIVER

3.1 On-Chip Antenna and Duplexer

There are three components shared by a CDMA transmitter and an FDMA

receiver in the RF-Front-End of Deadtime controller: an on-chip antenna, a duplexer, a

phase locked loop (PLL). As discussed, the important goal in this research is lowering

cost. To achieve this reducing external components and increasing efficiency using

more on-chip ones and combining common blocks are critical. Most wireless products

use external antennas. These are pretty big and occupy a large area in a printed circuit

board (PCB) especially when the ground plane area is included. An alternative solution

that can lower is an on-chip antenna fabricated in an integrated circuit using metal lines.

The study of on-chip antennas spans for over twenty years [20] - [25] and have shown

to be possible at frequencies as low as 5.8 GHz [26].

3.1.1 Overview of On-Chip Antenna

On-chip antennas have been fabricated in a the silicon substrate used in standard

CMOS technology. A die photo of dipole fabricated using a copper layer in UMC 130 nm

CMOS technology is shown in Figure 3-1. This dipole antenna is 3-mm long and has a

zigzag shape which can have higher gain than simple dipoles [27]. The copper layer

has 1.5-µm thickness and 30 µm widths, and there is an oxide layer with 3-µm thickness

between the metal layer and substrate.

A

Figure 3-1. On-chip antenna A) Die photo of an on-chip antenna fabricated using UMC 130nm CMOS technology B) Cross section of an on-chip antenna.

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Silicon Substrate(670 µm)

Oxide (3 µm)

Antenna

A

Figure 3-1. Continued

Figure 3-2. 3-mm zigzag antenna radiation pattern at 24 GHz [22].

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Figure 3-3. Antenna pair gain versus distance in the lobby of new engineering Building at 24 GHz. 3-mm on-chip zigzag dipole antennas fabricated on a 20−Ω−cm substrate with a 3-µm oxide layer are used for these measurements at 50-cm height from the ground [22]. The substrate thicknesses were 50, 100, and 670 µm.[22]

The measured data are shown in Figures 3-2 and 3-3. The former is an antenna

pair gain versus distance plot in the air with 3-mm long on-chip zigzag dipole antennas

with the substrate thicknesses of 50, 100, 670 µm. The latter is a radiation pattern.

Antenna pair gain is improved by thinning the substrate thickness by about 10 dB at 50

µm. The radiation pattern is consistent to that of a short dipole [22].

The environment of hybrid engine controller board is different from that of air

because there are many obstacles between chips. Some of them have pretty large

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height up to 2.5 cm. The antenna pair gain and radiation pattern will be changed in the

PCB boards because of these components. Some points selected to measure antenna

pair gain on the PCB board are shown in Figure 3-4.

Figure 3-4. Measurement points chosen on the PCB. Photo courtesy of Hainta Wu [28]

Antenna pair gain is defined as

( ) ( )2

rt222

211

221

a R4λGG

S1S1

SG

=

−−=

π (3-1)

Where Gt, Gr: the transmitting and receiving antenna gain

λ is the wavelength in free space

R is the distance between the antenna pair

The measurement results are shown in Figure 3-5.The substrate thickness is 670

µm. Each point represents the antenna pair gain between two points whose range is 6.5

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to 25 cm. The solid curve is the ideal one in free space based on Equation 3-1 at 24

GHz, assuming Gt and Gr are 0 dB. The maximum distance between a receiver and

transmitters is about 15 cm if the receiver of FDMA link is located on the center of board.

The sensitivity of FDMA receiver from table 2-2 is -74.3 dBm. The antenna pair gain

requirement is over -71 dB with 6 dB margin in real environment. Some are not

sufficient to meet the requirement. There are two ways to improve the antenna gain.

One is to decrease thickness of substrate and the other is to use a metal cover. The

measurements for the two cases are shown in Figures 3-5 [28].

Figure 3-5. Large scale fading channel measurement results. (11-15 means TX is placed at sampling point 11 and RX is placed at sampling point 15.) Theoretical value is calculated based on Friis formula and using the measured on-chip dipole antenna gains of -12 dB [28].

At all measurement points, up to 15 cm separation, the antenna pair gain is higher

than -68 dB. The implementation using an on-chip antenna should be possible based on

-85

-80

-75

-70

-65

-60

-55

-50

-45

w/ cover w/o cover theoretical value in the free space

4_5 1_3 1_3

1_3

1_3

4_5

1_2

1_2

1_2

5_6

5_6

5_6

4_7

4_7

4_7 6_7

6_7

6_7 6_7

12_14 11_13

12_14 11_13

12_14 12_14

11_13 11_13

11_15 11_15

11_15 11_15

8_9 8_9

8_9

8_9 8_9

2

2 14 RR

GGPP

rtt

r ∝

=πλ

f = 24 GHz, λ = 12.5 mm

5 10 15 20 Distance (cm)

8_10 8_10 8_10 8_10 8_10

Ga (

dB)

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these. An on-chip antenna is integrated with an FDMA receiver chain and a CDMA

transmitter in the UMC 130 nm logic CMOS technology.

3.1.2 Duplexer

Another block sharing a CDMA transmitter in the RF-Front-End is a duplexer.

SAW filters are used at frequency less than 3 GHz. But In this case, the operating

frequency is over 15 GHz. For the transceiver in the Deadtime controller, the duplexer is

composed of two third order band stop filters (BSF) as shown in Figure 3-6. There are

three ports: an antenna, a CDMA transmitter, and a FDMA receiver.

RXTX

Antenna

Duplexer

BSF BSF

Figure 3-6. On-chip duplexer using two band stop filters [29].

The operating frequency bands of CDMA link and FDMA link are 15.6 to 18 GHz

and 24.2 to 27 GHz. Base on these frequency allocations, the left BSF in Figure 3-6 has

a pass band from 15.6 to 18 GHz, and the right BSF has one at 24.2 to 27 GHz.

Looking at the specifications for each port of duplexer, insertion loss (IL) is below 3 dB

in the CDMA band, 15.6 through18 GHz, and in the FDMA band, 24.2 through to 27.2

GHz. Return loss (RL) is below 10 dB at each port in their respective pass bands.

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Isolation between TX port and RX port is better than 30 dB. These target requirements

are summarized in Table 3-1.

Table 3-1. Specification of the on-chip duplexer [29] Performance target

TX band (PA port) Insertion loss Below 3 dB for 15.6 ~ 18 GHz

Return loss Below 10 dB for 15.6 ~ 18 GHz

RX band (LNA port) Insertion loss Below 3 dB for 24.2 ~ 27 GHz

Return loss Below 10 dB for 24.2 ~ 27 GHz

Antenna port Return loss Below 10 dB for 15.6 ~ 18 GHz

and 24.2 ~ 27 GHz

PA and LNA Isolation

(Rejection)

Below 30 dB for 15.6 ~ 18 GHz

and 24.2 ~ 27 GHz

Figure 3-7. Schematic of the single-ended on-chip duplexer [29].

The schematic of single ended on-chip duplexer with two Chevyshev band stop

filters (BPFs) using three resonators with inductors and capacitors are shown in Figure

3-7. The band stop filter is used of a low pass filter (LFP) and a high pass filter (HPF).

PA LNA

Antenna TX side RX side

La1

Ca2

La3

Ca1

La2

Ca3

Lb1

Cb2

Lb3

Cb1

Lb2

Cb3

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For the transmitter side in Figure 3-2, La1, La2, and Ca3 form a low pass filter (LPF) and

Ca1, Ca2, and La3 form a high pass filter (HPF). A die photo of the single-ended on-chip

duplexer fabricated with an on-chop dipole antenna and a FDMA receiver is shown in

Figure 3-8.

Figure 3-8. Die photo of the single-ended on-chip duplexer.

3.2 Broadband Low Noise Amplifier

The first amplifying stage in the FDMA receiver is a low noise amplifier (LNA)

which needs high gain and wide bandwidth to lower noise figure and to cover the 3 GHz

bandwidth. Some studies have proposed for broadband LNAs [30]-[35]. A common way

is to cascade a few stages of LNA resonated at different frequencies. Another is to use

low quality factor (Q-factor) matching networks for input and output. Other is to use a

doubly-terminated LC ladder and a three section Chevyshev band pass filter for input

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matching, or shunt RC feedback. Some examples for achieving broad bandwidth are

shown in Figure 3-9.

Figure 3-9. Schematics of broadband LNA. A) Broadband LNA with low Q matching network [34]. B) LNA with a doubly terminated LC ladder [31]. C) LNA using three section Chevyshev band pass filter [32]. D) An LNA with shunt RC feedback [35].

The architectures in Figures 3-9 (B), (C), and (D) are usually used at frequencies

below 10GHz. Even though they have broad bandwidths of 3 to 10 GHz, their noise

figure is degraded at the higher end of band. For case (A) in Figure 3-9, the LNA has

about 10 dB of gain and less than 5 GHz bandwidth around 20 GHz. This gain is

modest due to low Q-factor matching networks. The gains of most circuits in the

literature do not exceed 15 dB of gain near 20 GHz [36]–[41]. An easy way to achieve

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higher gain is to cascade more stages. But this reduces bandwidth. To see this,

consider a block with unit DC gain and single pole response. The transfer function is

defined as

11)(+

=s

sHτ (3 - 1)

If n stages of such blocks are cascaded, the transfer function can be written as

n

ssH

+=

11)(

τ . (3 - 2)

Setting,

21

11)( =

+=

n

sjH

τω (3 - 3)

The 3-dB bandwidth is

121 1

3 −= ndB τ

ω (3 - 4)

As n goes to infinity, the overall bandwidth tends to zero. The equation 3-4 can be

approximately written using a series expansion of 1/21/n [42]

nnn

dB τττω 833.02ln11121 1

3 ≈≈−= (3 - 5)

From equation 3-5, the bandwidth decreases as square root of 1/n. Table 3-2

summarizes the bandwidth as function of n. For example, to implement an amplifier with

24 dB gain and 5 GHz bandwidth three amplifiers which have 8-dB gain and 10-GHz

bandwidth or four stages amplifiers which have 6-dB gain and 12-GHz bandwidth

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should be cascaded according to Table 3-2. It is challenging to achieve over 10-GHz

bandwidth near 20GHz.

Table 3-2. Bandwidth versus n [42]

n Actual

bandwidth(normalized)

Approximate

bandwidth(normalized)

Error

%

1 1.000 0.833 16.7

2 0.643 0.589 8.4

3 0.510 0.481 5.7

4 0.435 0.416 4.4

5 0.386 0.372 3.6

6 0.350 0.340 2.9

7 0.323 0.315 2.5

8 0.301 0.294 2.3

For more gain and wider bandwidth, a cascade of low noise amplifiers with varying

resonant frequencies is another candidate. A 5-stage gain distributed broadband

differential LNA is proposed and shown in Figure 3-10. It is composed of five cascode

common-source (CS) amplifiers with an inductive load and a source degeneration

inductor. Each amplifier is designed to have several dB gain and about 3-GHz

bandwidth. The loads of each stage are resonated at fc + 2.5 GHz or fc - 2.5GHz, and

input and output are matched to 50-Ω at fc.

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Figure 3-10. Schematic of 5-stages gain distributed broadband differential LNA.

Figure 3-11. Simple diagram and equivalent circuit of common source (CS) LNA. A) Simple CS LNA schematic B) Equivalent circuit of CS LNA.

Looking at the first stage of 5-stage gain distributed broadband differential LNA, it

is composed of an inductor for matching to 50-Ω and a CS LNA. A simplified CS LNA

topology is shown in Figure 3-11. The input impedance of CS LNA is

sgs

m

gssgin L

Cg

sC1)Ls(LZ

+++= (3 - 6)

The effective transconductance of the CS LNA is defined as

)R

Lω(1Rω

ω)Lω(RCω

gQgG

s

sTs0

T

sTsgs0

m1m1m

+=

+== , (3 – 7)

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where Q-factor of input network gs

mT

sgs0in C

gRC2ω

1Q 1, == ω (3 – 8)

If the input is matched to Rs,

)R

Lω(1Rω

ω)Lω(RCω

gQgG

s

sTs0

T

sTsgs0

m1m1m

+=

+== (3 – 9)

The effective transconductance can be written again as

=

0

T

sm ω

ωR

G2

1 (3 – 10)

The voltage gain of CS LNA is defined as

sgsgs

gssg

gs0

0

gs0

loadm

in

outv

RCQand

CLL

)Qωω

ωωj(2

)Qωω(Zjg

(ωV(ωVA

00

1

1)(

1where

))

ωω =

+=

−+==

(3 - 11)

If input is matched to Rs and Rs = ZLoad,

Load0

T

sLoadmv Z

ωω

RZGA

==

21

(3 - 12)

The overall gain of CS LNA can be varied between 3.5 to 8 dB because ωT/ω0 is in

the range between 3 to 5 [43].

A noise model of CS LNA is shown in Figure 3-12. There are three noise sources.

One is for the gate inducted noise (ig), another is channel thermal noise (id), and the

other is the source noise (vn). The output noise current is

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dgssgs

gssgg

sggs

sgn1 i

sC1ZZβZsC1ZZ

i1)Z(βZ1/sC

)Zβ(Zi

+++

+++

+++

+= (3 -13)

where β = ωT/jω

The noise factor is defined as [43]

( )

++−++=

T

0

gs

2gs

ind

gs

ωω

Q/5Q1δ5γδc2γ

QQ

1F1 (3 -14)

Zg

Zs

ig Cgsvn idβi i1= in1 + in2i

Figure 3-12. Noise model of CS LNA.

A cascode topology shown in Figure 3-13 is commonly used to improve the

stability, and increases isolation between input and output. Even though the noise

contribution of upper transistor M2 is often neglected at low frequencies for long channel

devices with high output resistance, it cannot be ignored around 20 GHz due to the

effects of drain-to-body capacitance. The noise factor for a cascode CS LNA is

1

22

21

2

1

5/4

WW

Q

5γδCc2γCFF

gs

rr

ββ

δ −+⋅== (3 -15)

Where β1 and β2 are the current gains and W1 and W2 are widths of M1 and M2.

Increasing the width of M2 makes β2 low and increases noise factor. Decreasing the

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width of M2 lowers the drain voltage of M1 and bias current which can bias M1 in the

linear region [43]. The optimal value of M2 is selected as the same as that of M1 [44],

[45].

c

- OUT +

c c

+IN -

Ls1 Ls2Lc

Ld1 Ld2

Cout1 Cout2

Cin1

Cin2

Cb1 Cb2

Figure 3-13. Schematic of differential common source (CS) amplifier with source degeneration inductor.

Figure 3-13 shows a stage of CS amplifier for the 5-stages gain distributed

broadband differential LNA. To increase common mode rejection ratio Lc resonated with

the parasitic capacitances of Ls1 and Ls2 is added. Source degeneration inductors are

added to the input transistors. Inductors used in the load and common node are

shielded using a polysilicon patterned ground shield to reduce loss.

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Figure 3-14. Simulation results of differential common source (CS) LNA. Overall gain and gain of each stage versus frequency

Figure 3-15. The S-parameter and noise figure simulation results of differential common source (CS) LNA.

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Figures 3-14 and 3-15 show the simulation results of the broadband LNA. The

overall gain is 25 dB at 30 GHz. It is over tuned in simulations to compensate the

expected down tuning in the actual silicon. It has 5.5 GHz bandwidth and about 4-dB

noise figure in simulations.

LNABalun Balun

AgilentE8361A PNA

50Ω50Ω

Figure 3-16. Measurement setup for 5 stage gain distributed differential LNA.

Figure 3-17. Characterization set up for Balun plus GSSG probe using a network analyzer.[46].

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A pair of Baluns (Krytar’s 180° Hybrid coupler) was used to convert single ended

to differential signal at the input, and to combine power of positive and negative nodes

of output in the measurement setup shown in Figure 3-17. To characterize the Balun

and GSSG probe, the reflection coefficients (Γin) are measured using Open, Short, Load

calibration structures. It is assumed that each port of Balun is matched to 50 Ω and

balanced between two 3dB ports. The operation frequency range of the Balun which is

6 to 26.5 GHz, however, limited the characterization of Balun because the phases of

two 3 dB ports are not balanced and matched to 50 Ω above 27 GHz. It is difficult to

characterize and get S-parameters of Balun and LNA. The balun complicates the

measurement S-parameters of LNA. It is much easier to measure LNA without Balun.

An alternative measurement setup is shown in Figure 3-18.

LNA

AgilentE8361A PNA

50Ω50Ω

Figure 3-18. Measurement setup for single ended mode.

It is challenging to make differential measurements using a two port Network

Analyzer without using Baluns. That means that it is challenging to measure differential

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components such as differential LNA using measurement setup in Figure 3-18. Even

though the measurement results are different from differential measurements, the LNA

was simulated in single ended and differential modes and characterized utilizing the

simulation result.

3GHz

A

6 dB

B

C

3 dB

D

Figure 3-19. Simulated S parameters and Noise Figure in single ended mode and differential mode A) S11 B) S21 C) S22 D) Noise Figure

The simulation results of single ended and differential mode are shown in Figure

3-19. In Figure 3-19 (A) S11 in single ended mode, the circuit is tuned at about 3 GHz

higher than in differential mode. The node which is connected with Lc in Figure 3-13 is

not AC Ground any more in the single ended mode. The input impedance of common

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source amplifier is described by Equation 3-6. There is no term related with Lc. which

must be included in the single ended mode. While |S22|’s of LNA in two modes are the

same. |S21| is 6 dB higher and Noise Figure is 3 dB lower in differential mode than these

in single ended mode.

Figure 3-20. Measured S-parameters in single ended mode.

3.3GHz

A B

Figure 3-21. Deembeded |S21| and noise figure of LNA A) |S21| B) noise figure

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A

B

Figure 3-22. Linearity measurement result of LNA A) IP1dB B) IIP3

Measurement results of LNA in single ended mode are shown in Figure 3-20 and

3-21. Intering the differential performance form single ended measurement, gain and

noise figure of LNA are achieved about 19 dB and 5.7 dB at 30.5 GHz with 3.3 GHz

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bandwidth. Input 1 dB compression point (IP1dB) is -30 dBm and input third order

intercept point (IIP3) is -18 dBm. The linearity measurement results are shown in Figure

3-22.

Table 3-3. Performance of LNAs over 20 GHz

Process Type fc (GHz)

Gain (dB)

NF (dB)

BW (GHz)

Supply Voltage

(V)

Power (mW)

[36] 0.13-μm

SOI CMOS

Differential 23.8 7.3 10 4.5 1.5 78

[37] 0.18-μm CMOS Single 21.8 15 6 NA 1.5 24

[38] 0.18-μm CMOS Single 23.7 12.9 5.6 2.5 1.8 54

[39] 0.18-μm CMOS Single 24 13.1 3.9 4.8 1 14

[40] 0.13-μm CMOS Differential 20 9 5.5 5.3 1.2 24

[41] 0.13-μm CMOS Single 26.2 8.4 5 3.7 0.8 1

This

Work* 0.13-μm

CMOS Differential 30.5 19 5.7 3.3 1.5 49.5

These are compared to the performance of LNA’s operating over 20 GHz in Table

3-3. Figure 3-23 shows a die photo of 5 stage gain distributed lose noise amplifier (LNA).

The die size is 980 µm by 430 µm.

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Figure 3-23. Die photo of common source (CS) LNA

3.4 Band Pass Filter

To select the signal in the desired band and to reject image during RF to IF

conversion, a band pass filter (BPF) is need before a mixer. The frequency plan of RF

to IF conversion in the FDMA receiver is shown in Figure 3-24. Images are located at

20.8 to 23.8 GHz when RF band is 24.2 through 27.2 GHz and local oscillator (LO)

frequency is 24-GHz. If there is no BPF, RF signal and Image are translated together to

the IF band. For the FDMA receiver, a 3rd order Chevyshev band pass filter (BPF)

shown in Figure 3-25 is chosen. It is composed of a pair of three resonators.

Figure 3-24. Frequency plan of RF to IF conversion

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L1 L3C1 C3

L2 C2

L2 C2

L1 L3C1 C3

Figure 3-25. Schematic of 3rd order Chevyshev band pass filter (BPF)

The simulation results of BPF are given in Figures 3-26 and 3-27. The insertion

loss (IL) is 3 dB and bandwidth is 6 GHz. The BPF is over tuned at 30 GHz like the LNA.

The S-parameter simulation results are shown in Figure 3-25 and phase versus

frequency plots are shown in Figure 3-27 for the ideal case (Ideal) using ideal LC

components and a more realistic case (Sim.) using LC components including parasitics.

Figure 3-26. S-parameter simulation results versus frequency of 3rd order Chevyshev

band pass filter (BPF) A) |S21| and |S11| versus frequency. B) S11 versus frequency

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Figure 3-27. Simulated phase versus frequency of 3rd order Chevyshev band pass filter (BPF) with ideal LC components and LC components including parasitics

Figure 3-28. Die photograph of 3rd order Chevyshev band pass filter (BPF)

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3.4 Broadband RF Amplifier

A second broadband amplifier is added between the BPF and mixer. A three

stages gain distributed cascode broadband RF amplifier uses the same topology as the

5-stage LNA. Each stage is tuned at fc - 2.5-GHz, fc, and fc+2.5-GHz as shown in Figure

3-29, and input and out are tuned at 30 GHz in simulation to compensate the expected

down tuning in silicon like that was down for the design of the low noise amplifier and

the bandpass filter. The measurement setup and deembeding techniques are the same

as LNA. The measurement results are shown in Figures 3-30 through 3-34.

Figure 3-29. Schematic of a 3-stages gain distributed cascode RF amplifier (RFA)

Figure 3-30. S parameter measurement results of a 3-stages gain distributed cascode RFA and a bandpass filter in single ended mode

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A

Figure 3-31. Measured |S21| in single ended mode and deembeded one in differential mode of a bandpass filter and a RFA

Figure 3-32. Measured noise Figure in single ended mode and deembeded one in differential mode of a bandpass filter and a RFA

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A

B Figure 3-33. Linearity measurement results of bandpass filter (BPF) and RFA

combination A) IP1dB B) IIP3

The deembeded gain of bandpass filter and RF amplifier combination is 5.2 dB

with 3.2 GHz bandwidth at 30 GHz in differential mode. The expected gain of RFA is

about 9 dB based on simulations with bandpass filter loss of 4 dB. The noise figure of

two components is 11.4 dB in differential mode. IP1dB is -16 dBm and IIP3 using two tone

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at 30 and 30.001 GHz is -6 dBm. The die photo of 3 stage gain distributed amplifier is

shown in Figure 3-34.

Figure 3-34. Die photo of a 3-stages gain distributed cascode RFA

3.5 Broadband Down Conversion Mixer

A mixer translates frequency in a wireless system. The carrier frequency of

received signal is translated using multiplication with a local oscillator (LO). For LO

signals, square wave is generally used instead of sine wave because the former

renders mathematically 2 dB higher conversion gain [47]. A mixer can be classified as a

passive and an active mixer. An active mixer is used for the FDMA receiver. A simple

single balanced active CMOS mixer and the functional representation are shown in

Figure 3-35. It is composed of three parts. One is a transconductance stage (M1) to

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convert voltage to current, another is a switching stage (M2 and M3), and the other is a

load (two RL’s).

Figure 3-35. Single-balanced mixer. A) schematic B) functional representation for the large switching signals

When RF input is VB + vRF, where VB is the dc bias voltage and vRF is the small signal

RF input voltage, the output current through the left load resistor in Figure 3-35 (A) is

defined as [48]

)v21V(t),VF(I RFBLOo1 += (3 -16)

Assuming that vRF is small, Equation 3-16 can be approximately rewritten using a Taylor

series as

.22

RFm1B

RFB

BLOBLOo1

(t)vg(t)I

v21

V)V(t),VF()V(t),VF(I

+=

∂∂

+≅

(3 -17)

Similarly, the output current of other side is

22RFm1B

o1(t)vg(t)II −≅ (3 -18)

Therefore, total output current is

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RFm1oo1o (t)vgIII ≅−= 2 (3 -19)

Including LO input signal, if the products from the high order harmonics of LO signals

are ignored, the output voltage is approximately [49]

−+−

−= )tωcos(ω

21)tωcos(ω

21

π4ARg(t)outV LORFLORFLm1 (3-20)

Filtering the High frequency term,

)tωcos(ω21

π4ARg(t)outV LORFLm −

−= 1 (3-21)

Conversion gain is

RgvA Lm2

1 (3-22)

For a single balanced mixer, the switching pair acts like as differential amplifier during

portions of operation, and square wave LO signal appear in the spectrum. To remove

the undesired output LO components, a double balanced mixer in Figure 3-36 is used

[50].

Figure 3-36. Double balanced Gilbert cell mixer

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gm1 and gm2 are the transconductance of MR1and MR2. The output current through MR1

and MR2 from Equation 3-19 are

RFmgmoRFm1gmo (t)vgI(t)vgI 22,1, , == . (3 -19)

In the case of 50% duty cycle, where TLO is a period of square wave

)T(tgg LOmm 212 += (3 -20)

The overall current is

RFeffRFmm1gmogm1oo (t)vgv(t)g(t)gIII =−=−= )( 22,, . (3 -21)

The output voltage of mixer is

RFeffL

gmogm1oL

out (t)vgRIIRV2

)(2 2,, −=−−= . (3 -22)

Conversion gain of double balanced mixer can be written as

(t)gRA effL

v 2−= . (3 -23)

The real square wave, however, is not perfect. It has finite slope in the rise and fall

transitions. When the transition time is ∆t and gm0 is the magnitude of gm1 and gm2,

conversion gain can be approximately rewritten as [51]

.2

)sin(2mo

L

LO

LOv gR

tftfA ⋅⋅

∆⋅∆⋅

⋅≈ππ

π (3 -24)

The noise generation in the mixers is complicated since the operating point of

device is changed periodically with time. Noise comes from the transconductor stage,

switching stage, and load [50]. Looking at the noise from the transconductor stage, the

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power spectrum density (PSD) of the drain thermal noise of MOS transistor in saturation

region is

mgkTf

i γ42

=∆ , (3 – 25)

where gm is transconductance, k is the Boltzmann’s constant, T is absolute temperature,

and γ is 2/3 for long channel devices, and can be higher for short channel devices. For

the square wave in LO signal case, the thermal noises of drive stage (M1 in Figure 3-35,

MR1 and MR2 in Figure 3-36) in the odd harmonic frequencies of LO signal are down

converted to IF because a square wave is composed of odd harmonics of the

fundamental. These noises are not correlated. The noise from fLO ± fIF, from 3fLO ± fIF,

and rest of higher order harmonics are 81%, 9% and 10% respectively (Figure 3-37)

[52].

Figure 3-37. Frequency translation of white noise in transconductor stage

For a single balanced mixer, PSD is

21

11

01 )(4)( m

mgsn g

grRkTfS γα ++= (3 – 26)

For a double balanced mixer when gmR1 = gmR2 and rg1 =rg2, PSD is

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21

11

012 )22(4)( mR

mRgRsnR g

grRkTfS γα ++= (3 – 27)

The second noise source is the thermal noise generated in the switching pair. If

transistors M2 and M3 in Figure 3-35 are assumed to be in saturation region during ON,

the output current determined by tail current and M1 and M2 does not contribute noise. If

LO is sufficiently high, this noise is smaller than that of drive stage. If both M2 and M3

are ON, they cause noise. The instantaneous noise PSD at output port (Io1) is

+

=32

3202 4)(

mm

mmn gg

ggkTfS γ . (3 – 27)

Because the noise at one port is twice of Io1, the corresponding output noise PSD is

.2)(where

),(816)(

32

32

32

32023

+

=

=

+

=

mm

mm

mm

mmn

ggggtG

tgGkTgg

ggkTfS γγ

(3 – 28) [52]

G(t) is the small signal transconductance. As the amplitude of LO increases, the interval

time when both M2 with M3 are on decreases and the noise decreases (Figure 3-35).

Time averaging the PSD at output,

.2where

,8)(18)(0

023

o

B

T

LOn

VIG

GgkTdttGT

kTfS LO

π

γγ

=

=

= ∫

(3 -29)

The PSD of noise at the output is proportional to the bias current and inversely

proportional to the zero crossing slope of LO signal.

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Figure 3-38. Time varying transconductance of the switching pair and the PSD of generated thermal noise [52]

The third noise source is the LO port. Even though it is very complicated because

the LO is a periodically time varying and the noise at the output contains cyclostationary

components. Simplifying the LO port as the time invariant stationary voltage noise

source, output noise is

)()()( tntGty LOnLO = , (3 -30)

where G(t) is the time varying transconductance of the switching pair (M2 and M3 in

Figure 3-35) and nLO(t) is noise at LO port. For a single balanced mixer, PSD of noise

from LO port is

( )dttG

TG

GrRkTfS

LOT

LO

gLOnLO

∫=

+=

0

22

22

0

)(1where

24)( γ

. (3 -31)

RLO is the equivalent noise resistance at LO port. The external noise at LO port,

however, is rejected in a double balanced Gilbert cell mixer. The PSD for this is

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22

0 )4(4)( GrkTfS gnLO γ= . (3 -32)

Including the three noise sources and that generated by loads, single side band (SSB)

noise factor (F) [52] is

sm

LgLOmmg

SSBSB RgcR

GrRGggr

cF 2

12

2211111

2,

1)2(2)( +++++=

γαγα

(3 -33)

For a double balanced mixer, noise factor is

sMRm

LMLgMRmMRmMRgMR

SSBDB RgcR

GrGggr

cF 2

1,12

21,11,11,1,1

2,

144)(2 +++++=

γαγα

(3 -34)[52]

Figure 3-39. Schematic of double balanced Gilbert cell mixer with source degeneration inductors

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The schematic of double balanced Gilbert cell mixer with source degeneration

inductors for the FDMA receiver is shown in Figure 3-39. The basic architecture shown

in Figure 3-36 is augmented to improve the performance. Like in the LNA, source

degeneration inductors (LS1 and LS2) are added to improve linearity, LS3 is added to

improve common mode rejection resonating the parasitic components at the common

mode node. LD1 is added for noise rejection from the LO port by resonating the parasitic

components at the drain nodes of MR1 and MR2. Even though the inductor loads are

usually used for GHz IF, resistive loads are used to increase bandwidth. The simulation

results of mixer are in Figures 3-40, 3-41 and 3-42.

Figure 3-40. Voltage gain versus intermediate frequency (IF) as function of load resistance

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Figure 3-41. Voltage gain and power gain versus input power

Figure 3-42. Noise figure versus intermediate frequency (IF) as function of load resistance

Voltage conversion gain is -4.5 dB, 3-dB bandwidth is 4.5 GHz, and noise figure

is 12.8 dB at If of 1.5 GHz with -6 dBm Local Oscillator (LO) power. In Figure 3-41

power gain is greater than the voltage gain. The conversion voltage gain of mixers is

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normally higher than power gain. This, however, depends on the input and load

impedances. The relationship between power gain and voltage gain is

Z1Re

Z1Re

2V

Z1Re2v

Z1Re2v

PP P

in

LGAIN

inin

Lout

in

outGAIN =

×

×== (3 – 35)

If the input and load impedance are the same, power gain is the same as voltage gain.

If Re1/ZL is higher than Re1/Zin, then the power gain is higher than the voltage gain.

Figure 3-43 shows a die photograph and layout of the mixer.

A B Figure 3-43. Die photograph and layout of broadband double balanced Gilbert cell

mixer A) Die photograph B) Layout

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CHAPTER 4 INTERMEDIATE FREQUENCY TO BASEBAND CONVERSION

4.1 IF-to Baseband Conversion System

The second down conversion stage that frequency translates from intermediate

frequency (IF) to baseband (BB) is shown in Figure 4-1. The stage is composed of three

parts. One is a broadband IF amplifier with over 3-GHz bandwidth. Another is seven

mixers that convert IF signals to baseband signals with seven different intermediate

frequencies. The other is an intermediate frequency generator using the 24 GHz signal

from a phase locked loop (PLL). This can simultaneously generate seven different

signals with frequencies at 0.4, 0.8, 1.2, 1.5, 2.0, 2.4, and 3.0 GHz. According to the

original frequency plan, there were two other IF frequencies at 1.6 GHz instead of 1.5

GHz and 2.8 GHz instead of 3.0 GHz. These allocations are changed to simplify the

structure of IF generator. This is allocated since there is a great deal of flexibility for

frequency allocation in a self contained system enclosed by a conductive case.

FrequencyGenerator

PLL

24GHz

.

400 MHz

.

.

.

.

CH1

CH2

CH7

800 MHz

3 GHz

400MHz800MHz

3GHz

IFAMPIF

CH6

2.4 GHz

Figure 4-1. Block diagram for IF to baseband conversion

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The bandwidth of received signal in the FDMA link is 3 GHz from 200 MHz to 3.2

GHz. This is an extremely wide IF range. Amplifiers with an inductive load are usually

used several gigahertz. The bandwidth of those is too narrow to cover the 3-GHz range.

For the FDMA receiver, an amplifier with resistive feedback is used at IF. It can cover a

wider band and is simple. The down conversion mixer needs also broad bandwidth to

cover whole the entire band. A double balanced mixer using a Gilbert cell and resistor

load is used to decrease second harmonic effect and to increase the bandwidth. The

seven mixers have the same structure and size. It is not easy to simultaneously

generate the LO signals at multiple frequencies. Frequency synthesizers in a

communication system with multiple channels like ultra wideband (UWB) system

multiply or divide using mixers to generate LO signals at a wide range of frequencies.

This requires more space and filters. Alternate way is to use only buffers and D Flip-

flops. This can be compact because it does not need any inductors and capacitors

which occupy large space. Each block in IF to Baseband conversion and baseband

circuit are explained in this chapter.

4.1.1 Intermediate Frequency Amplifier

There are many reports for a wide band amplifier used in broad band systems like

UWB [53] - [58]. A simple amplifier architecture for several-GHz systems is an inverter

with resistive feedback [59], [60] between input and output. Schematic of the proposed

two stage IF amplifier is shown in Figure 4-2. Both NMOS and PMOS transistors form

the amplifier. The DC bias at input and output is set by a feedback resistor. A separate

bias circuit is not needed. A capacitor is used for DC blocking between the amplification

stages. The bandwidth of inverter with resistive feedback is determined by the RC time

constants at the input and output nodes [60].

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Figure 4-2. Schematic of broadband IF amplifier with resistive feedback

A schematic of single stage resistive feedback amplifier and its equivalent circuit

are shown in Figure 4-3.

Figure 4-3. Schematic of single stage of resistive feedback inverter and equivalent circuit A) Schematic of inverter amplifier with resistive feedback B) Equivalent circuit of the amplifier

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The loop gain is defined as

21

121 )////1//()(

ZZZrr

sCZZgT opon

dsm +

+= , (4 -1)

where gm = gmn + gmp; and gmn and gmp are the transconductances of NMOS and PMOS

transistors.

Cds = Cdsn + Cdsp; where Cdsn and Cdsp are the drain-source capacitance of NMOS

and PMOS transistors.

Z1 = 1/s(Cgsn + Cgsp); Cgsn and Cgsp are the gate to source capacitance of NMOS

and PMOS transistors.

Z2 = Rf /(1+ Rf s(Cgdn + Cgdp); Cgdn and Cgdp are the gate-to-drain capacitance of

NMOS and PMOS transistors.

Open loop gain is

1

2

ZZA −=∞ (4 -2)

and the closed loop gain is

TAT

/11+= ∞

(4 -3)

If Z1 is greater than Z2 and the gate-to-source capacitance and gate-to-drain

capacitances are neglected, the transfer function of single stage inverter with resistive

inverters is

)( 11 −− ++−=

oponds

m

in

out

rrsCg

VV

. (4 -4)

If the source resistance is RS, the noise figure (NF) of the amplifier is [61]

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f

ssm

Tf

s

ssm RRRg

ff

RR

RRgNF +⋅++⋅+≈

32)()1(1

321 2

2 (4 - 5)

And the input impedance is

v

Lfin A

ZRZ

++

≈1 (4 - 6)

Where opondsL rrsCZ ////= .

If the source resistance is small, the gain of resistive inverter becomes

)( fsmin

outv RRg

VVA +== . (4 - 7)

In simulations, the two stage resistive feedback inverter has 18 dB gain at 1.6 GHz,

3.3 dB noise figure, and 3.3 GHz 3-dB bandwidth. The layout is shown in Figure 4-4 and

its size is 220 µm by 250 µm. This is fabricated in the UMC 130nm CMOS technology.

Figure 4-4. Layout of a differential IF amplifier with resistive feedback

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4.1.2 IF to BB Down Conversion Mixer

There are signals at seven different FDMA channels. They should operate at the

same time. The total bandwidth of them is 3 GHz. To support the wide bandwidth from

200 MHz through 3.2 GHz at the input, a Gilbert cell mixer with resistive loads is used.

To reduce the effect of even order harmonics, a double balanced structure is used. It is

straight forward to use differential topology because the FDMA receiver is fully

differential.

CH1

CH2

CH3

CH4

CH5

CH6

CH7

0.4 0.8 1.2 1.6 2.0 2.4 3.0 GHz

IF : 0.4 0.8 1.2 1.5 2.0 2.4 3.0GHz

0

IFA

IF : 0.4 , 0.8, 1.2, 1.5, 2.0, 2.4, 3.0GHz

Figure 4-5. Frequency plan of IF to BB conversion

The mixer in Figure 4-7 is a simple heterodyne down conversion mixer. To look

at the frequency conversion scheme, input signal is define as

tARF RFRFinput ωcos= (4 - 8)

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and if LO is set as

)cos( θω += tLO RF , then (4 - 9)

baseband out is

[ ])]2cos([cos21

)cos()cos(

θωθ

θωω

++=

+=

tAA

ttABB

RFRFRF

RFRFRFouyput

(4 - 10)

Filtering the high frequency term with a low pass filter, and amplifying the signal with

gain of 2, the output is

θcosRFouyput ABB = . (4 - 11)

Figure 4-6. Zero IF down conversion scheme using simple homodyne architecture

Another possible solution for this is to use Hartley architecture shown in Figure 4-7.

It needs two mixers, two 90-degree phase rotators and a combiner to recover signal and

to reject image. Equations from 4-11 to 4-13 show how RF signal is converted to

baseband and recovered.

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LPF

cosωRFt+ϴRFin

π/2

IF π/2

BBout

cosωRFtΣ

XA1(t) XA2(t)

XB1(t) XB2(t)LPF

Figure 4-7. Zero IF down conversion scheme using Hartley architecture

[ ]

θ

θωθ

θωω

cos21)(

)2cos(cos21

)cos(cos)(

2

1

RFA

RFRFRF

RFRFRFA

AtX

tAA

ttAtX

=

++=

+⋅=

(4 - 11)

[ ]

θ

θωθ

θωω

cos21)(

)2sin(sin21

)sin(cos)(

2

1

RFB

RFRFRF

RFRFRFB

AtX

tAA

ttAtX

=

++=

+⋅=

(4 - 12)

θ

θθ

cos

cos21cos

21)()()( 22

RF

RFRFBAout

A

AAtXtXtBB

=

+=+= (4 - 13)

We need seven mixers. The Hartley is more complicated and requires more area.

A simpler architecture is preferred in multiple channel systems. The simpler one is

selected for the FDMA receiver. There is, however, a problem in these architectures. If

θ = 90º there is no signal in baseband because cos(90º) is zero. This well known nulling

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problem for AM systems should be fixed to recover the signals at baseband. The

simplest way is to use LO signals which have phase significantly away from 90 degrees.

This can be accomplished by generation of two LO phases and selecting the one that

results higher baseband output. There are a few ways to generate the phases [62]-[64].

A RC low pass filter or gm-C is usually used to generate the phases. Some use digital

like delay cells with D flip-flops. This needs reference signal with 50% duty cycle and a

specific divider ratio like 2, 4, 8, 16, etc. In the IF LO generator used in this research, it

is challenging to make two signals with phase difference of the 90 degrees at every

output frequencies especially without significantly increasing the chip area. Instead, The

IF generator outputs two signals with phase differences between 60 and 90 degrees.

How to generate the two signals will be discussed in next chapter. Another requirement

is the duty cycle of IF LO signals. They must have 50% duty cycle. Such a signal has

only DC and odd harmonics of the signal at fundamental frequency. Square wave with

50% duty cycle and a period (T0) is shown in Figure 4-8.,

Figure 4-8. Square wave with 50% duty cycle

Using the complex exponential Fourier series, a physical waveform can be

represented over the interval a < t < a +T0 [65]

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∑∞=

−∞=

=n

n

tjnnectW 0)( ω

(4 – 14)

Where the complex Fourier coefficients cn is

dtetWT

c tjnTa

an0

0 )(1

0

ω−+

∫= (4 – 15)

and ω0 = 2πf0 = 2π/T0.

For the square wave in Figure 4-5, the complex Fourier coefficients are

)1(2

10

0 2/

00

−== −−∫ πω

πjntjnT

n en

AjdteAT

c , (4 – 16)

where A is the amplitude of square wave.

Using l’Hospital’s rule,

=

=−

=

=

evenn

oddnnAj

nA

cn

,0

,

0,2

π (4 – 17)

From equation 4-17, there is no even harmonics in the square wave. The complex

Fourier coefficients can be represented using sync function in frequency domain as

2/)2/sin(

22

πππ

nneAc

jn

n

= (4 – 18)

The power spectrum density (PSD) of square wave with 50% duty cycle is shown

in Figure 4-9.

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Figure 4-9. Power spectral density (PSD) of square wave with 50 % duty cycle

If the duty cycle is not 50 %, however, the complex Fourier coefficients are changed and

some of them are not zero when n is even. For example, when the duration of HIGH is

T0/2 + ∆t, the complex Fourier coefficients are

)1(2

100

0

22/

00

−⋅== −∆−

−∆+

∫ ππ

ω

πjnT

tnjtjntT

n een

AjdteAT

c (4 – 19)

Comparing equation 4-19 with 4-16, there is a new term with ∆t.

=+−

=+−

=∆

+

=

∆−

∆−

evennenAj

oddnenAj

nT

tA

c

Ttnj

Ttnj

n

),1(2

),1(2

0),21(2

0

0

2

20

π

π

π

π (4 – 20)

When ∆t = (1/8)T0, C0 = (5/8)A, C1 = [(1- j)/2π]A, and C2 = [(-1+ j)/4π]A. The

second harmonic has a finite value. This causes a mixer to have an even order

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harmonic problem and degrade the linearity of a mixer. So IF generator should make all

the outputs to have 50% duty cycle. Some frequencies whose divider ratio at the end is

2N when N is an integer, 50% duty cycle is obtained by the divider. For other outputs,

duty correction circuits are required. An intermediate frequency generator composed of

divider chains and duty correction circuits will be discussed in the next chapter.

LO+ LO+

LO-

RF+ RF-

Figure 4-10. Schematic of double balanced Gilbert cell mixer

Figure 4-10 shows the schematic of a double balanced Gilbert cell mixer

integrated in the FDMA receiver. The mixer has two load resistors. These are formed

using poly resistors with a silicide block that has higher sheet resistance and lower

temperature coefficient. In the double balanced structure, the mismatch of load and

MOSFETs cause even harmonic problems that degrades linearity. To reduce the

mismatch in the load several resistors are connected with parallel instead of one and

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dummy resistors are added on both sides of resistors to decrease the variations. The

layout is drawn to keep symmetry.

Even though the FDMA receiver needs seven, only one is fabricated for the test

purpose. In the test structure, each IF LO signal from IF generator is selected by a 3-

bits decoder. The layout of a mixer fabricated in the UMC 130-nm CMOS technology is

shown in Figure4-11. The size of mixer cell is 42 µm by 52 µm.

Figure 4-11. Layout of double balanced Gilbert cell mixer

4.2 Baseband Architecture

There are three parts in the baseband section for each channel of the FDMA

receiver as shown in Figure 4-12: a low pass filter, a baseband amplifier, and a

comparator. Since there are seven channels in the FDMA receiver, seven baseband

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links are needed. The architecture and specification of components in the baseband is

the same for all channels.

Figure 4-12. Block diagram of baseband section of the FDAM receiver

The first stage is a low pass filter (LPF). When the IF mixer frequency translates,

one agian there are signals at fc-fIF and fc+fIF. The filter is used to reject the high

frequency term and to select the low frequency one. The proposed LPF structure is

shown in Figure 4-13. The low pass filter is composed of a source follwer and an RC

filter.

Figure 4-13. Schematic of the third order low pass filter

The third order low pass filter has 270-MHz bandwidth and 3 dB of loss in

simulation. The layout of LPF integrated in the FDMA receiver is shown in Figure 4-14.

The layout size is 84 µm by 65 µm in the UMC 130 nm logic CMOS technology.

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Figure 4-14. Layout of the third order low pass filter

Figure 4-15. Schematic of 3-stage baseband amplifier.

A baseband amplifier is composed of three stages of basic cells shown in Figure

4-15. A basic cell is a differential amplifier with common mode feedback using a resistor

(R2). The output dc bias is set by R2 and the gain of a basic cell is set by R1 and R2.

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Gain of each stage is R2/R1 and set to 5 dB. The total voltage gain of amplifier is 15 dB.

The bandwidth is 250-MHz which is sufficient to cover the 150 MHz of signal bandwidth.

The layout of baseband amplifier is shown in Figure 4-16 and its size is 150 µm by 32

µm.

Figure 4-16. Layout of the baseband amplifier

Figure 4-17. Schematic of comparator and SR latch

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The last stage of receiver is a one-bit comparator composed of two single to

differential amplifiers with wide bandwidth and an SR latch that is composed of two

NOR gates to convert sinusoidal signal to square wave. The comparator determines the

high and low levels of incoming signals. The schematic of amplifier and block diagram

of comparators and SR latch are shown in Figure 4-17. The layout is shown in Figure 4-

18. The comparator size is 47 µm by 74 µm.

Figure 4-18. Layout of comparator and SR latch

4.3 Measurement Results

The measurement scheme, setup, chip, a Printed Circuit Board (PCB), and a

bonding diagram for the mixer are shown in the Figure 4-19. Looking at the

measurement setup, the two inputs, IF and LO signals are injected from signal

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generators using a GSSG probe and a Balun. The Input signal is a single tone which

has 10 to 50 MHz higher frequency than the frequency of IF LO signal. The outputs of

mixer are connected to an external operational amplifier (AD8138, Analog Device) with

6 dB gain and a voltage divider to drive a spectrum analyzer with 50-Ω input impedance.

Figure 4-19. Measurement setup and test structure of the mixer and baseband amplifier integrated with an FDMA receiver A) Measurement setup B) Die photo of test structure C) Test PCB board D) Block diagram of test structure E) Zoomed in photo of bonding area

Figure 4-20. Input measurement scheme of IF to BB converter test structure

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Figure 4-21. Measurement setup and PCB board of IF to BB converter test structure

Figure 4-22. Measurement results of IF to baseband conversion stage A) Gain and frequency response of each channel at baseband B) Gain versus intermediate frequency

The output of mixer and baseband amplifier are connected to an external

operational amplifier (OPA) with high input impedance for converting differential signal

to single ended for testing. In Figure 4-22, the two plots show the gain and frequency

response of each channel versus baseband frequency (A) and gain of each channel

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versus intermediate frequency (IF) (B) for the IF to baseband conversion stage. The IF

amplifier and mixer have 10 MHz of bandwidth. This is currently limited by an external

amplifier. The gain of the IF amplifier and mixer combination channels 1 to 7 have 23.6,

27.5, 27.6, 25.6, 23.3, 23.1, and 21.5 dB.

Figure 4-23. Measurement results of LPF and baseband amplifier A) Frequency response at baseband B) Gain of the LPF and BB amplifier

The measured characteristics of low pass filter (LPF) and baseband amplifier

(BBA) are shown in Figure 4.23. As mentioned, the baseband amplifier has 250 MHz

bandwidth and 15 dB of gain, and the low pass filter has 250-MHz bandwidth and 3-dB

loss in simulation. In Figure 4-23, measured gain is 5 dB, bandwidth is about 40 MHz

and power consumption is 1.5 mW. The gain is degraded by 7.5 dB in the

measurements. Since the load resistance of baseband amplifier is 18kΩ while input

resistance of external operational amplifier used for measurements is 5kΩ. This reduces

gain to 1/3 of simulation or by 7 dB. If this loss is de-embedded, gain of the low pass

filter and a baseband amplifier combination is about 12 dB. The bandwidth is still small.

This appears to be caused from the parasitic capacitance of line and pad for connecting

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the external load. To fix this problem, the external amplifier AD8138 was replaced with

an AD 8131ed for the subsequent effort.

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CHAPTER 5

SYNTHESES OF MULTIPLE INTERMEDIATE FREQUENCIES

5.1 Background of Frequency Generation

As discussed, a key challenge is generating LO signals at multiple frequencies for

channel selection. It is not practical to use multiple voltage controlled oscillators

(VCO’s) to synthesize because they occupy a large area and consume much power.

Approaches to synthesize multiple frequencies for ultra wideband systems have been

suggested [66]-[68]. These normally have complicated architecture and cannot

simultaneously output signals at multiple frequencies. To make the system compact, the

proposed multiple LO generator uses only transistors except for the 12 GHz and 24

GHz buffers. This frequency generator frequency divides the 24 GHz signal from s

phase locked loop (PLL) and simultaneously generates seven frequencies using static

frequency dividers [69] [70]. The generated frequencies and divide ratios for each

channel are listed in Table 5-1.

Table 5-1. Intermediate frequency and frequency divider ratio Signal Frequency Generation

LORef 24 GHz LC-VCO + PLL

IF1 0.4 GHz LOR/2/2/2.5/2/3

IF2 0.8 GHz LOR/2/2/2.5/3

IF3 1.2 GHz LOR/2/2/2.5/2

IF4 1.5 GHz LOR/2/2/2/3

IF5 2.0 GHz LOR/2/2/3

IF6 2.4 GHz LOR/2/2/2.5

IF7 3.0 GHz LOR/2/2/2

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Potentially, a lot of dividers are needed. Simplification is required to decrease size,

and power consumption. This can be achieved by sharing dividers. Such simplification

is shown in Figure 5-1.

Figure 5-1. Simplified frequency generation scheme

Based on Table 5-1, potentially twenty six dividers are need. If dividers are shared,

the number of dividers can be reduced to nine. In the original frequency plan, 2.8 GHz

and 1.6 GHz are used for channel 3 and channel 7. 2.8 GHz is replaced with 3.0 GHz

because generation of 2.8 GHz is not easy using only dividers. It requires a mixer and a

filter as shown in Figure 5-2. 1.6 GHz is replaced with 1.5 GHz because generation of

1.6 GHz requires a divide-by-1.5 circuit. It is difficult to make the output to have 50 %

duty cycle. To generate 1.5 GHz, the 3.0 GHz output needs to be simply frequency

divided by two.

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Figure 5-2. Generation of 2.8 GHz using a mixer and a high pass filter (HPF)

5.2 Frequency Generation and Duty Correction

Looking at Table 5-1 and Figure 5-1, seven divide-by-2, a divide-by-3, a divide-

by-2.5 are needed to support the seven necessary output frequencies. The divide-by-2

circuit using a D flip-flop (DFF) is straight forward. There are two latches in the DFF

forming the master and slave. The input of DFF is connected to the inverted output and

the input signal is fed to the clock port (Figure 5-3 (A)). The schematic of current mode

logic (CML) static divide-by-2 based on a D-type flip-flop (DFF) is shown in Figure 5-3

(B). It can operate over a wide frequency range (> 20 GHz) and has moderate power

consumption comparing to the dynamic one [70].

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A

B

Figure 5-3. Schematic of current mode logic (CML) static divide-by-2 based on a D flip-flop [70] A) Block diagram of divide-by-2 circuit. B) Schematic

The second divider is the divide-by-2.5 circuit. Its divide ratio is fractional. In the

case that a divide ratio is x.5, where x is an integer, the divider architecture is similar to

the one with divide ratio of 2x+1. The only difference is the use of dual edge triggered

flip-flops for a fractional divider instead of using single edge (either rising or falling edge)

triggered flip flops. A divide-by-2.5 circuit was implemented with three dual edge

triggered flip flops and a NAND gate as shown in Figure 5-4. A duty correction circuit to

change the duty ratio to 1:1, however, is required to reduce the even order harmonic

output. Without it, the duty ratio of outputs is 3:2 or 2:3.

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D1 Q1 Q2 Q3

OUT(3:2)

CLK

D QQ

D QQ

D QQ

CLK

D1

Q1

Q2

Q3

Figure 5-4. Block diagram and waveforms of a divide-by-2.5

2.4 GHz Q1 Q1_dOUT

12 GHz

D QQ

D QQ

12 GHz

6 GHz

OUT

12 GHz

2.4 GHz

2.4 GHz

(/2)

(Q1)

(Q1_d)

3 : 2

1 : 1

1/2.4GHz (416.7ps)

(41.7ps)1/24GHz

Figure 5-5. Duty cycle correction scheme for the divide-by-2.5 and waveform to generate 2.4 GHz output

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The duty correction circuit for the 2.4 GHz output is composed of two dual edge

triggered flip-flops (DEDFFs) and an AND gate. Q1 and Q1_d delayed by 41.7-ps which

is a half period of 12-GHz through a DEDFF in Figure 5-5. The product of two 2.4 GHz

waveforms can make output with a 1:1 duty cycle using an AND gate.

OUT

CLK

D QQ

D QQ

1:1 Input Duty Ratio

3:2 Input Duty Ratio

IN

OUT

IN

OUT

1 : 2

3(37.5%) : 5(62.5%) 2(28.6%) : 5(71.4%)

Figure 5-6. Block diagram and waveforms of a divide-by-1.5 circuit

A divide-by-1.5, which is another fractional divider, is made of two dual edge

triggered D flip flops and a NOR gate shown in Figure 5-6. This has a duty cycle

problem like the divide-by-2.5 circuit. The duty cycle ratio of output is 1:2 when the input

duty cycle ratio is 1:1. The output duty cycle is 3:5 and 2:5 when the input duty cycle is

3:2. The duty correction circuit uses the 1:1 input duty cycle case. The duty correction

circuit for the 1.6 GHz LO signal is shown in Figure 5-7. The Q1_d which is a delayed

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signal of Q1 by a quarter of an input clock signal period (156.25 ps) is needed. None of

the outputs of dividers have such phase. The delay is generated using a combination of

analog delayers. Because of this, the circuit is susceptible to variations.

Figure 5-7. Duty correction scheme for the divide-by-1.5 and waveforms

A divide-by-3 circuit using D flip-flops generally provides output with 3:2 or 2:3 duty

cycle ratio. For 800-MHz and 2.0 GHz LO signal generation, a divide-by-3 and duty

correction circuits are need. An approach to implement these is shown in Figure 5-8.

This circuit is composed of two D flip-flops (DFF), one latch, one AND gate, and a

multiplexer. Two DFFs (FF0 and FF1) and an AND gate (G0) are for divide-by-3 in the

upper side and a latch and a multiplexer in the lower part are for duty correction.

Looking at waveforms Q1 and Q2 which are delayed by a half cycle of reference clock

(CK) using a latch (LT0) either, generates the CLK3 with a 1:1 duty cycle ratio in

conjunction with a multiplexer that chooses either in Q1 and Q2.

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Figure 5-8. Block diagram and waveforms of a divide-by-3 [71]

Another solution uses three dual edge triggered flip-flops (DEFFs) as shown in

Figure 5-9. It does not need any additional components for duty correction. Even though

a DEFF is bigger than a single edge triggered flip-flop, it has the advantage to provide a

1:1 duty cycle ratio. Because it uses both rising and falling edges, it can divide with a

fractional ratio with only three DEFFs. For 0.4, 1.2, 1.5, and 3.0 GHz outputs, they do

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not need duty correction circuit because the last divide stage that generates the signals

has a divide ratio of 2, which makes the output duty cycle ratio 1:1.

Q1

OUT

CLK

Q2

Q3

Q1 Q2 Q3 OUT

CLK

D QQ

D QQ

D QQ

Figure 5-9. Block diagram and waveforms of a divide-by-3 circuit using three dual edge

triggered flip-flops (DEDFFs)

5.3 Phase Generation

The other requirement of LO generation is providing two output phases with an

offset larger than 60 °. The phases which IF generator supports are listed in Table 5-2.

As mentioned in the previous chapter, 90-degree phase offset is desired, but in some

case, it is not straightforward to generate them. This depends on the duty cycle of input

and divide ratio. If the input duty cycle is 50% for divide-by-2 circuit, there is no problem

generating signals with the 90 degree phase offset. For the other cases when the divide

ratio is 2.5 or 3, this is not straightforward.

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Table 5-2. Phases difference generated by IF generator according to frequencies Signal phase

3.0G 90°

2.4G 72°

2.0G 60°

1.5G 90°

1.2G 90°

0.8G 60°

0.4G 90°

CLK

Q1

Q2

T4

3T4

Figure 5-10. Waveforms of a divide- by-2 circuit

Starting with divide-by-2 circuit, both Q1 and Q2 in Figure 5-10 are the frequency

divide-by-2 waveforms of input (CLK). Q1 is divided at the rising edge, while Q2 is done

at the falling edge. The time difference is T/4 which is 90 degrees in phase. One of them

is selected by a multiplexer.

For the second case, 2.4-GHz output generates two signals with zero and 72

degree phase. In Figure 5-4, there are three dual edged triggered flip-flops (DEDFFs) in

the divide-by-2.5 output. They delay each output of the previous stage by a half of

period of input. For example, Q2 is delayed signal of Q1 by a DEDFF in Figure 5-11.

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The delay time is 1/5 period of output with frequency that is two and half divide by the

frequency, which corresponds to 72 degrees.

CLK

D1

Q1

Q2

Q3

T5

4T5

Figure 5-11. Waveforms of a divide-by-2.5

Q1

OUT

CLK

Q2

Q3

T6

5T6

Figure 5-12. Waveforms of a divide-by-3

The last case for 800 MHz and 3.0 GHz which use divide-by-3 circuit is shown in

Figure 5-12. Q2, Q3 and OUT in Figure 5-12 are the outputs of three DEDFFs.

Comparing Q3 with OUT, the latter is delayed by a half period of input (CLK). It is 1/6

period of output, or the phase difference between Q3 and OUT is 60 degrees.

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5.4 Measurement of Test Structure

The test structure for IF generator is fabricated in the UMC130nm CMOS

technology. It generates seven frequencies (0.4, 0.8, 1.2, 1.5, 2.0, 2.4, and 3.0 GHz)

using 12 GHz input. The test structure also includes an output buffer and a multiplexer

to select the output channel for IF generation circuit and another output buffer and 100

MHz generation circuit including divide-by-60 circuits for trigger an oscilloscope for

Phase offset measurements. The function for frequency selection and phase selection

scheme is summarized in Table 5-3.

Table 5-3. Frequency and phase selection

Channel FS2 FS1 FS0 HL

0.4GHz 1 1 0 0/1 (90°)

0.8GHz 1 0 1 0/1 (60°)

1.2GHz 1 0 0 0/1 (90°)

1.5GHz 0 1 1 0/1 (90°)

2.0GHz 0 1 0 0/1 (60°)

2.4GHz 0 0 1 0/1 (72°)

3.0GHz 0 0 0 0/1 (90°)

The layout size of test structure for IF generation is 783 by 720 µm2. The layout,

die photo, printed circuit board (PCB) and measurement setup are shown in Figures 5-

13 through 5-15. The input at 12 GHz from a signal generator and the output frequency

was measured with a spectrum analyzer. The duty cycle was measured with an

oscilloscope. The phase offset between two selectable signals of each channel was

measured using 100MHz triggering signal.

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A

B Figure 5-13. Measurement scheme and Die photograph of IF generator A)

Measurement scheme and layout B) Die photograph

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Figure 5-14. Printed Circuit Board (PCB) of IF generator testing

Figure 5-15. Measurement setup for IF generator testing

Signals with seven different frequencies from 400 MHz to 3 GHz were generated

by the IF LO generation circuit. One of them can be chosen using a 3-bit selector in the

test structure. The measured output spectra of each channel are shown in Figure 5-16.

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A

B

C

D

Figure 5-16. . Output spectra of IF generator A) 400 MHz B) 800 MHz C) 1.2 GHz D) 1.5 GHz E) 2.0 GHz F) 2.4 GHz G) 3.0 GHz

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E

F

G

Figure 5-16. Continued

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A B

C D

E F

Figure 5-17. Measured duty cycle ratio of output waveforms of IF generator in the Oscilloscope Agilent® infiniium 86100B A) 400 MHz single ended B) 400 MHz differential . C) 800 MHz single ended D) 800 MHz differential E) 1.2 GHz single ended F) 1.2 GHz differential G) 1.5 GHz single ended H) 1.5 GHz differential I) 2.0 GHz single ended J) 2.0 GHz differential K) 2.4 GHz single ended L) 2.4 GHz differential M) 3.0 GHz single ended N) 3.0 GHz differential

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G H

I J

K L

M N

Figure 5-17. Continued

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The duty cycle and phase offset between two selectable signals of each channel

are measured using an oscilloscope (Agilent® infiniium DCA 86100B). The output

waveforms are shown in Figure 5-17. The duty cycle of the each channel is 49.4 %

(400MHz), 48.5 % (800MHz), 46.4 % (1.2GHz ), 54.4 % (1.5GHz), 53.9 %(2.0GHz),

54.9 % (2.4GHz), 48.2 % ( 3.0 GHz) for single ended measurements and 49.5 %

(400MHz), 49.6 % (800MHz), 49.2 % (1.2 GHz), 50.1 % (1.5GHz), 49.3 %(2.0GHz),

50.2 % (2.4GHz), 50.4 % (3.0 GHz) for differential measurements . The deviation is less

than ±5 % in the single ended case, while that is less than 0.5 % for differential case.

A B

Figure 5-18. Measured output waveforms of 400 MHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH

A 100-MHz signal was used as a trigger signal and as the reference to measure

phase offset between two selectable signals of each channel. The 400 MHz waveform

in Figure 5-18 (A) lags the triggering signal by 835 ps when the selector signal for phase,

HL_SEL is LOW, when HL_SEL is HIGH, the waveform in Figure 5-18 (B) lags

triggering signal by 1.465 ns. The time difference of two 400MHz signals in Figures 5-18

(A) and (B) is 630 ps, which is 25.2 % of a period of 400 MHz which is 2500 ps. The

corresponding phase offset of 400MHz output is 90.7° more slightly.

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°=°⋅= 7.903602500630

pspsoffsetPhase (5 – 1)

Using the same way the phase offsets of other channel can be calculated from

waveforms. The phase offset of 800 MHz output is 59.9° from Equation 5-2 and Figure

5-19.

°=°⋅−

= 9.593601250

)500708(ps

psoffsetPhase (5 – 2)

A B

Figure 5-19. Measured output waveforms of 800 MHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH

The phase offset of 1.2 GHz output is 93.3° from Equation 5-3 and Figure 5-20.

°=°⋅−

= 3.9336033.833

)636852(ps

psoffsetPhase (5 – 3)

A B Figure 5-20. Measured output waveforms of 1.2 GHz and 100 MHz trigger signal A)

HL_SEL = LOW B) HL_SEL = HIGH.

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The phase offset of 1.5 GHz output is 90.7° from Equation 5-4 and Figure 5-21.

°=°⋅−

= 7.9036067.666

)229397(ps

psoffsetPhase (5 – 4)

A B

Figure 5-21. Measured output waveforms of 1.5 GHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH

The phase offset of 2.0 GHz output is 64.8° from Equation 5-5 and Figure 5-22.

°=°⋅−

= 8.64360500

)318408(ps

psoffsetPhase (5 – 5)

A B

Figure 5-22. Measured output waveforms of 2.0 GHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH

The phase offset of 2.4 GHz output is 72.6° from Equation 5-6 and Figure 5-23.

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°=°⋅−

= 6.7236067.416

)73157(ps

psoffsetPhase (5 – 6)

A B

Figure 5-23. Measured output waveforms of 2.4 GHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH

The phase offset of 3.0 GHz output is 83.2° from Equation 5-7 and Figure 5-24.

°=°⋅−

= 2.8336033.333

)268345(ps

psoffsetPhase (5 – 7)

A B

Figure 5-24. Measured output waveforms of 3.0 GHz and 100 MHz trigger signal A) HL_SEL = LOW B) HL_SEL = HIGH

The measured phase offset are close to the target for the output except the ones at 2

and 3 GHz whose error is about 8 %.

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A B

C D

E F

G H

Figure 5-24. Measured Phase Noise of each channel and input reference signal A) 400 MHz B) 800 MHz C) 1.2 GHz D) 1.5 GHz E) 2.0 GHz F) 2.4 GHz G) 3.0 GHz H) 12 GHz input reference

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The phase noise of outputs was measured using Agilent® E4448A Spectrum

Analyzer. The phase noise 12 GHz input is -131.1 dBc/Hz of at 1MHz offset. The

measurement results are shown in Figure 5-25 and summarized in Table 5-4. The

power consumption of IF generation block is 90 mW, but including the power

consumption of a 24-GHz buffer from the PLL, the total is 106 mW.

Summary

Table 5-4. Summary of IF generator measurement

Channel Duty cycle ratio (%) Phase

Offset (Target)

Phase Noise @ 1MHz (dBc/Hz) Single Ended Differential

0.4 GHz 49.4 49.5 90.7° (90°) -144.5

0.8 GHz 48.5 49.6 59.9° (60°) -144.4

1.2 GHz 46.4 49.2 93.3° (90°) -140.0

1.5 GHz 54.4 50.1 90.7° (90°) -140.8

2.0 GHz 53.9 49.3 64.8° (60°) -136.6

2.4 GHz 54.9 50.2 72.6° (72°) -139.7

3.0 GHz 48.2 50.4 83.2° (90°) -136.2

In this chapter, an intermediate frequency LO generator circuit that simultaneously

generates multiple signals with different frequencies is proposed and the measurement

results are presented. The circuit generates seven outputs at frequencies; 0.4, 0.8, 1.2,

1.5, 2.0, 2.4, and 3.0 GHz. Each output has two selectable phases. The output

frequencies were checked from 0.4 to 3 GHz with an oscilloscope and a spectrum

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analyzer. The output duty cycle variation is less than ± 5% in single ended

measurements and ± 1% in differential measurements. The phase offset of two

selectable signal of each channel was measured using a 100-MHz triggering signal. The

deviation of offset for target is less than 8 %. Phase Noise of each channel was

measured with a 12-GHz input signal.

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CHAPTER 6 FDMA RECEIVER CHARACTERIZATION

6.1 Test Structure

The full architecture of FDMA receiver in the controller section of the hybrid engine

controller board was shown in Figure 2-2. There are seven mixers and seven baseband

chains for the seven channels. This increases the chip size. The fabricated test

structure of receiver is shown in Figure 6-1.

Figure 6-1. Test structure of FDMA receiver

Only one baseband chain is included. It is a simpler way to test a channel even

though it is not possible to support multiple channels at one time. To select an

appropriate channel during the IF to baseband conversion, an 8-to-1 multiplexer is used

to select the necessary Local Oscillator (LO) signal. Another buffer is added to drive the

mixer. As described in chapter 5, the IF generator synthesizes signals at seven different

frequencies (0.4, 0.8, 1.2, 1.5, 2.0, 2.4, and 3.0GHz) with two selectable phases. Only

one IF to baseband conversion and a baseband chain composed of an IF amplifier, a

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mixer, a LPF, a baseband amplifier, and a comparator are taped out as part do the

FDMA receiver test structure. The test scheme and measurement setup are illustrated

in Figure 6-2. The output of mixer and baseband amplifier are connected to an external

operational amplifier (OPA) with high input impedance for converting differential signal

to single ended one for measurements.

A

Figure 6-2. Test scheme and measurement setup of FDMA receiver A) Test scheme and PCB B) Measurement setup (C) Chip (D) PCB (E) Power and spectrum analyzer setup

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Figure 6-3. Die photo of transceiver at Deadtime controller

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6.2 Measurements of FDMA Receiver Chain

6.2.1 RF Front-End Measurements

Duplexer LNA BPF RFA

SignalGenerator

Balun

50Ω

SpectrumAnalyzer

Balun

50Ω

FDMA Receiver

RF input

RF output

Figure 6-4. Measurement scheme for RF Front-End of FDMA receiver

The blockdiagram shown in Figure 6-4 is the measurement setup for the first three

components: Low Noise amplifier (LNA), Band Pass Filter (BPF) and RF amplifier (RFA).

There is separated test structure for this. Instead, this is measured in the receiver chain.

The RF amplifier is connected to a Pad and the RF-to IF down conversion mixer. This

means measurement results are different from them in the receiver chain. In simulation,

the power gain is degraded by 3 dB when the output of RF amplifier is connected to a

50 Ω load. The loss of cable, probe and Duplexer should be considered to estimate the

gain of RF-front-end of FDMA receiver. The measurement results of Duplexer which

was measured by Hsinta Wu [72] are shown in Figure 6-5. Based on them, the gain is

calculated and the plot is shown in Figure 6-6.The maximum gain is 22 dB at 30 GHz.

While the passband of FDMA receiver is 24.2 through 27.2 GHz. The expected

frequency down tuning is not observed. The lowest frequency band of seven channels

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in FDMA receiver has about -20 dB of gain and the highest one of them has 5 dB of

gain.

Figure 6-5. Measurement results of Duplexer for Antenna and FDMA receiver ports [72]

Figure 6-6. Gain of RF-Front-End of FDMA receiver

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6.2.2 RF-to-Baseband Converter measurements

LNA BPF RFA IFA BBALPF Comparator BUF

SignalGenerator

Balun

50Ω

RF input

PLL

IFGEN

BUF

MUX

24 GHz

0.4 – 3 GHz

SpectrumAnalyzer

AMP

750Ω

750Ω

1.5KΩ

1.5KΩ

50Ω

+-

AD8131

SpectrumAnalyzer

AMP

750Ω

750Ω

1.5KΩ

1.5KΩ

50Ω

+-

AD8131

FDMA Receiver

SignalGenerator

93.75 MHz

Figure 6-7. Measurement setup of IF to BB Down conversion

The measurement setup for IF-to-Baseband down converter is shown in Figure 6-

7. The outputs of IF-to-BB mixer and baseband amplifier can be measured in this setup.

To transfer RF signal to baseband, a phase locked loop (PLL) provides the 24 GHz LO

signal to RF-to-IF down conversion Mixer and IF generation circuit which synthesizes

seven LO signals from 400 MHz to 3 GHz for IF-to BB Mixer. Even though the IF

generator can simultaneously synthesize seven different LO frequencies, as discussed

only one of them is used to convert IF signal to baseband to select one channel.

The frequency of RF signals for each channel is 10 MHz higher than the center

frequency of each channel. This means that the RF signal of every channels converted

down to 10 MHz at the baseband. The outputs of IF-to-BB Mixer and baseband

amplifier (BBA) for seven channels when the RF input power is -50 dBm are shown in

Figure 6-8. To increase the bandwidth of external operational amplifier, AD 8131, is

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replaced with AD8138. The input Impedance of AD8131 is too small comparing to the

output impedance of IF-to-BB mixer and baseband amplifier. In simulations, the gain of

IF-to-BB Mixer decrease by 12 dB and one for BBA drops by 27 dB. The gain plot of

LNA to baseband amplifier after deembeding the effect of external operational amplifiers

is shown in Figure 6-7. The highest gain of 40 dB from LNA to Baseband amplifier is

observed at RF input frequency of 30 GHz. The lowest one of 13 dB is measured at RF

frequency of 24.4 GHz. Mistuning the RF-front-end causes the gains to vary with

channel.

A B

C D

Figure 6-8. Measured output power of IF-to-BB Mixer and Baseband amplifier (BBA) with -50 dBm RF input power for each channels A) Mixer output with 24.41 GHz input B) BBA output with 24.41 GHz input C) Mixer output with 24.81 GHz input D) BBA output with 24.81 GHz input E) Mixer output with 25.21 GHz input F) BBA output with 25.21 GHz input G) Mixer output with 25.51 GHz input H) BBA output with 25.51 GHz input I) Mixer output with 26.01 GHz input J) BBA output with 26.01 GHz input K) Mixer output with 26.41 GHz input L) BBA output with 26.41 GHz input M) Mixer output with 27.01 GHz input N) BBA output with 27.01 GHz input

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E F

G H

I J

K L

M N Figure 6-8. Continued

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Figure 6-9. Gain of LNA to Baseband amplifier of FDMA receiver

LNA BPF RFA IFA BBALPF Comparator BUFBalun

50Ω

RF input

PLL

IFGEN

BUF

MUX

24 GHz

0.4 – 3 GHz

OscilloscopeAMP

750Ω

750Ω

1.5KΩ

1.5KΩ

50Ω

+-

AD8131

Oscilloscope

FDMA Receiver

SignalGenerator

93.75 MHz

SignalGenerator

BERT

SignalGenerator

50 Mbps Data

4 GHz

23 GHz

AMP

Figure 6-10. Measurement setup for ASK modulated data of FDMA receiver

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Agilent® N4906A Serial Bit Error Tester (BERT) is used to generate PRBS or

specific data patterns for ASK modulation. Data from BERT is used to modulate a 4-

GHz carrier. The modulated signal was upconverted to 27 GHz using an external mixer

and a 23-GHz signal source. The spectrum of modulated signal with PRBS data at 27

GHz is shown in Figure 6-11. As explained a previous chapter, one of seven

frequencies synthesized by IF generator can be chosen using an 8-to-1 multiplexer. The

LO signal at 3 GHz is selected for the data at 27 GHz. The modulated RF input signal is

down-converted to baseband and output waveforms are checked using a

oscilloscope( Agilent® 54831D) . Another external amplifier is used in this measurement

setup because the output of mixer needed amplification for use with oscilloscope.

Figure 6-11. Spectrum of ASK modulated PRBS data

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A B

Figure 6-12. Output waveforms of IF-to BB Mixer and ones of Inverted input data with 50 Mbps data rate A) 1110 1100 Pattern B) PRBS data

The output waveforms of IF-to-BB Mixer are show in Figure 6-12. Comparing to

the inverted input data pattern, the output data patterns are the same as the input in

specific and PRBS patterns. Finally the output of FDMA receiver is converted to Digital

signal by a comparator and an SR latch. Inverter buffers drive load. The output

waveforms of FDMA receiver converted to digital data are shown in Figure 6-13. The

waveforms are compared with inverted input data pattern, and they are the same.

A B

Figure 6-13. Output waveforms of FDMA receiver and ones of Inverted input data with 50 Mbps data rate A) 111110000 B) 1110011000

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Figure 6-14. Noise Figure measurement result of FDMA receiver

A Figure 6-15. Linearity measurement result of FDMA receiver A) IP1dB B) IIP3

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B Figure 6-15. Continued

Noise Figure and Linearity measurement results are shown in Figures 6-14 and 6-

15. Noise Figure of 27 GHz channel is 8.7 dB. For RF frequency below ~ 26 GHz, the

noise figure exceeds 10 dB. ) IP1dB – 29 dBm and IIP3 is -20dBm with 27.01and 27.011

GHz. The total power consumption of FDMA receiver is 242.3 mW including that for the

PLL. FDMA test structure works for a single channel even though the total gain of each

channel is not sufficient comparing to the target due to the frequency mistuning in the

RF-front-end. Redesign of RF-front-end Is needed for proper operation.

6.2 Time Shared FDMA Receiver

The FDMA receiver needs seven IF-to-Baseband conversion stages to support

seven channels. This will significantly increase the chip area. To make the receiver

compact, alternate architecture is proposed. More specifically, the time shared FDMA

receiver shown in Figure 6-16 is proposed.

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Figure 6-16. Block diagram of time shared FDMA receiver architecture

A time shared FDMA receiver architecture which requires a single IF to baseband

converter and a baseband chain is shown 6-16. To the FDMA receiver test structure in

Figure 6-1, two more blocks are added as shown Figure 6-16. One is a 3-bit counter to

provide selector signals to the 8-to-1 multiplexer and the other is a Parallelizer which

converts the incoming serial data to parallel data.

Figure 6-17. Channel selection scheme of time shared FDMA receiver

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An 8-to-1 multiplexer (MUX) selects an LO signal with required intermediate

frequency, and provides it to the mixer according to the selector signal from the counter.

Since the counter provides periodic 3 bit selector signal to the 8-to-I MUX, each channel

is converted at t1 to t7 slots in a period as shown in Figure 6-17. The baseband signal is

converted to parallel data using a 1-to-7 serial to parallel converter shown in Figure 6-18.

Since the data of seven channels are allocated in series, parallelized data at each are

that for each channel. To enable to this, the mixer and baseband section should have

sufficient time to settle to support the input data rate (50Mbps). Another test board

shown in Figure 6-19 including the counter and 1-to 7 serial to parallel converter in

Figure 6-18 is built. This is used in conjunction with PCB board shown in Figure 6-2.

DFF

DFF

DFF

DFF

DFF

DFF

DFF

DFF

DFF

DFF

DFF

DFF

DFF

DFF

3-bitCounter

Data

SignalGnenerator

CLK1X

CLK7X

CH1

CH2

CH3

CH4

CH5

CH6

CH7

Figure 6-18. Block diagram of 1-to-7 serial to parallel converter

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3-bitSelector

FDMARX test PCB

FDMARX

Serializer

Parallelizer

3-bitCounter

Data

CLK7XCLK1X Signal

Gnenerator

Figure 6-19. Test plan with two PCB board for the time shared FDMA receiver

LNA BPF RFA IFA BBALPF Comparator BUFBalun

50Ω

RF input

PLL

IFGEN

BUF

MUX

24 GHz

0.4 – 3 GHz

OscilloscopeAMP

750Ω

750Ω

1.5KΩ

1.5KΩ

50Ω

+-

AD8131

Oscilloscope

FDMA Receiver

SignalGenerator

93.75 MHz

SignalGenerator

DigitalPattern

GeneratorSignal

Generator

24 GHz

AMP

SignalGenerator

SignalGenerator

3-bit Selector

Data1

Data2

Data3

fLO2

fLO1

fLO3

PowerCombiner

Figure 6-20. Test structure of time shared FDMA receiver for three channels

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The test scheme of time shared FDMA receiver for three channels is shown in

Figure 6-20. It is a little different from the initially proposed measurement setup in which

a 3-bit counter is used to produce 3-bit selector signals for a 8-to-1 multiplexer (MUX). A

digital pattern generator replaced with 3-bit counter for selector and the serialized data

can be checked in an oscilloscope. For this setup, however, five signal generators are

needed. Due to the number of available signal generators, the measurements have

been done for only two channels. A BERT which has two data port, DATA and DATAB,

was used for data pattern generation instead of a digital pattern generator and one bit

selector signal was used.

Figure 6-21. Waveforms of test structure of time shared FDMA receiver for two channels

To check the waveform easily in an oscilloscope, simple data patterns shown in

Figure 6-21 are used. From a pair of input data pattern, CH1 and CH2, one of them is

chosen alternatively by SEL signal. The data rate of selector is twice as fast as one of

data. When SEL is LOW the data from Channel 1 is selected, while the data from

Channel 2 is chosen when SEL is HIGH. For measurements, a pair of 26 GHz and 27

GHz channels and a pair of 25.5 GHz and 26 GHz channels were selected.

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A B

Figure 6-22. Output and selector waveforms of test structure of time shared FDMA receiver for two channels A) IF-to BB Mixer output B) Buffer output

Data rate of input pattern for Channel 1 and Channel 2 is 10 Mbps and the selector

signal rate is 20 Mbps. The output waveforms of IF-to-BB mixer and buffer measured

using an oscilloscope are shown in Figure 6-22. Comparing to the waveforms in Figure

6-21, the measured output pattern is the same as expected, illustrating that the time

shared FDMA receiver properly works. This architecture, however, can work up to 10

MHz selection rate currently instead of 350 MHz selection rate needed for the system.

The time shared FDMA receiver should be measured using seven channels .

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CHAPTER 7

SUMMARY AND SUGGESTED FUTURE WORKS

7.1 Summary

An FDMA receiver architecture with an IF LO generator that synthesizes seven LO

signals for wireless interconnection on a hybrid engine controller printed circuit board is

proposed.

A broadband low noise amplifier and RF amplifier at 30GHz are implemented. A

3rd order Chevyshev band pass filter is included in the RF front-end. The RF mixer

utilizes a double balanced Gilbert cell topology and supports 3 GHz bandwidth. For IF to

baseband conversion, an IF amplifier with resistive feedback and a broadband down

conversion mixer are implemented.

For generating the seven LO signals for the IF-to-baseband conversion, a

frequency divider based approach is chosen. The seven LO signals are generated by

dividing 12-GHz 50% duty cycle signal. Duty cycle correction circuits are included to

make the duty cycle of all the outputs 50%. The generator also provides two outputs

with phase shift greater that 60 ° to mitigate the AM nulling problem.

A full FDMA receiver test structure from antenna to baseband section, and a test

structure of IF generator are implemented (Figure 6-1), and their operation is

demonstrated. The gain of receiver chain from LNA to Baseband amplifier is 40 dB and

noise figure is 8.7 dB at 27 GHz about 242.3 mW of power consumption.

A time shared FDMA receiver architecture including an FDMA receiver, a 3-bit

counter and a 1-to-7 serial to parallel converter is presented. The feasibility for a time

shared FDMA receiver architecture is suggested.

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7.2 Suggested Future Work

(a) Currently, the main problem of FDMA receiver Is that it does not have sufficient

gain in the target frequency range because the components of RF front-end including

the low noise amplifier (LNA), bandpass filter (BPF) and RF amplifier (RFA) are tuned

around 30 GHz. For better performance, the RF-front-end should be retuned for

operation at 24.2 though 27.2 GHz.

(b) A full FDMA receiver test structure was characterized for gain, noise figure,

linearity, and functionality. A Bit Error Rate (BER) test is suggested to experimentally

determine the sensitivity.

(c) The proposed time shared FDMA receiver was measured with only two

channels. The system for hybrid engine controller board needs to simultaneously

support seven channels, and should be tested with all the channels.

The initial scheme using external control circuits for time sharing on a separate

board could not handle all the channels. The time sharing function should be integrated

with the receivers on the same chip.

(d) The FDMA receiver was characterized. The FDMA transmitter was built by

Kyujin Oh [73]. The operation of FDMA receiver with the FDMA transmitters should be

demonstrated.

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BIOGRAPHICAL SKETCH

Minsoon Hwang was born in Onyang, Korea, in 1976. He received the B.S. degree

in electronics engineering from Chungam National University, Daejeon, Korea in 2001

and M.S. and Ph.D. degree in electrical and computer engineering from University of

Florida, Gainesville, Florida in 2004 and 2011. He joined the Silicon Microwave

Integrated Circuits and Systems (SiMICS) research group since 2007.

He worked on call processing software design of base station of CDMA 2000 for

LG Electronics Inc. in 2000- 2001 and high speed I/O driver using differential signaling

such as Low Voltage Differential Signaling (LVDS), Reduced Swing Differential

Signaling (RSDS), min-LVDS, Point to Point Differential Signaling (PPDS) for Flat

Panel Display (FPD) for LG Electronics in 2004-2006. His current research interest is in

analysis and design of RF circuits, wireless transceiver and mixed mode circuit design

in CMOS.