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K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

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Page 1: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

K-Band Focal Plane Array:Integrated Downconverter Module #1

Matt Morgan and Tod Boyd

National Radio Astronomy Observatory

8/7/2008

Page 2: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1 is Complete

Page 3: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM2 is Not Complete – One Key Part Missing

I mistakenly ordered the wrong size feedthru header for this module. They havebeen re-ordered, and are expected to arrive in mid-September.

Page 4: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured Gain

The bandpass is a little narrow. I will show later that it is not the filter.I probably just need to raise the lid slightly.

Page 5: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured Gain

IF Response shows a lot of ripple. I believe this is related to cavity effects onthe PCB-side – which will not be present on IDM2.

Page 6: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured Image Rejection

Image rejection at ±1.2-3 GHz offsets is better than 35 dB.

Page 7: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured Image Rejection

Image rejection at ±5.9-7.7 GHz offsets is better than 32 dB.

Page 8: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured Gain Compression

Output 1 dB compression point is about +7 dBm.

Page 9: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured LO Power Requirements

Page 10: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured Channel Isolation

There seems to be excessive crosstalk between channels (-20 dB), havinga strong IF dependance, but virtually no RF/LO dependance – this stronglysuggests that the crossover is occuring in the IF circuit inside the PCB cavity.

Page 11: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured Return Loss

Poor return loss needs investigation.

Page 12: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured Return Loss

Poor return loss needs investigation.

Page 13: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

IDM1: Measured Return Loss

Poor return loss needs investigation.

Page 14: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

Probe Measurements on Filters

Dynamic range of the measurement was limited at the high frequency end,but the passband looks perfect.

Page 15: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

Probe Measurements on Filters

Perfect.

Page 16: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

Compliance Matrix for Single Pixel Prototype

parameter symbol spec/predicted measurement comments

noise temperature Te 600 – 800 K not measured

gain G 30 dB 30 dB

gain ripple Gmax – Gmin 3 dB 8 dB presumed PCB cavity effect

output power Pout -25.5 0.5 dBm

-25.5 0.5 dBm

assuming predicted front-end gain

headroom HR +40 dB +33 dB probably ok

LO1 power required

PLO1 -3 5 dBm +1 8 dBm

LO2 power required

PLO2 +3 5 dBm +3 5 dBm

image rejection IR 25 dB 32 dB

channel isolation Iso 30 dB 20 dB presumed PCB cavity effect

return loss RF input

IF output

LO1 input

LO2 input

-17 dB

-19 dB

-12 dB

-10 dB

-11 dB

-11 dB

-6 dB

-12 dB

need to verify transition designs

mass M 250 g 316 g IDM2 will be much less, average should still meet spec

Page 17: K-Band Focal Plane Array: Integrated Downconverter Module #1 Matt Morgan and Tod Boyd National Radio Astronomy Observatory 8/7/2008

Future IDM1 Revisions

1. Modify ALH444 bias circuit for better gain repeatability.

2. Modify PCB cavity to include a metal barrier between IF circuits in bothchannels – this should improve channel isolation and IF gain flatness

3. Investigate cause of return loss problems – may require re-design ofthe transitions

4. Raise the lid above the filters to prevent de-tuning.

5. Clean up other minor PCB issues