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Folie 1 Analog Filtering Reinhard Keller This is a little overview of what is done and what is planned against RFI with analog filters at the Effelsberg Telescope. Folie 2 Bonn, 30. March 2001 RFI Mitigation Workshop 2 Analog Filters are everywhere In the frontends: at RF stages at IF stages at DC In the backends at IF level at DC Besides many classical filters a lot of shielding is used to avoid RFI. That is what industry calls EMC, electro-magnetic compatibility. Filters are also incorporated in the DC connectors.

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Folie 1

Analog Filtering

Reinhard Keller

This is a little overview of what is done and what is planned against RFI with analogfilters at the Effelsberg Telescope.

Folie 2

Bonn, 30. March 2001RFI Mitigation Workshop2

Analog Filters are everywhere

In the frontends:– at RF stages

– at IF stages

– at DC

In the backends– at IF level

– at DC

Besides many classical filters a lot of shielding is used to avoid RFI. That is whatindustry calls EMC, electro-magnetic compatibility. Filters are also incorporated in theDC connectors.

Folie 3

Bonn, 30. March 2001RFI Mitigation Workshop3

RFI at 21cm in Effelsberg:

The need of RFI mitigation is obvious! Small bands are reserved for astronomy butwideband observation are wanted. Only a few interferers are known. Most of themare changing with time and also in frequency. This delimits hardware filtering

Folie 4

Bonn, 30. March 2001RFI Mitigation Workshop4

Fixed Filters:

Frequency domain: – Bandpassfilter

– Bandstopfilter (Notch)

(Time domain)

Folie 5

Bonn, 30. March 2001RFI Mitigation Workshop5

Fixed Frequency Filters

Before LNA:1. Avoid saturation

(„robust receiver“)

2. Select desired frequencies

→ low loss → high gain stability

After LNA:1. Select desired

frequencies

2. Avoid saturation(„robust receiver“)

→ high selectivity → high gain stability

Folie 6

Bonn, 30. March 2001RFI Mitigation Workshop6

Fixed Frequency Filters

are

simple

Need no info about RFI

but

Seperation of RFI ⇔ signal in frequency domain

Folie 7

Bonn, 30. March 2001RFI Mitigation Workshop7

Example 1: 1.9cm Receiver

Realized at the Effelsberg telscope

Folie 8

Bonn, 30. March 2001RFI Mitigation Workshop8

13 GHz High Pass Filter

-80

-60

-40

-20

0

10 12 14 16 18 20

f/GHz

S/d

B

Folie 9

Bonn, 30. March 2001RFI Mitigation Workshop9

13 GHz High Pass Filter

Insertion loss S21-Betrag

-0.5

-0.4

-0.3

-0.2

-0.1

0

10 12 14 16 18 20

f/GHz

S/d

B

Folie 10

Bonn, 30. March 2001RFI Mitigation Workshop10

13 GHz High Pass Filter

waveguide realization:

Folie 11

Bonn, 30. March 2001RFI Mitigation Workshop11

„Adaptive“ analog filters

Switched filters:– Realized in Effelsberg

Prooved, but after LNA!

Tunable filters: – Waveguide filters;

Mecanicaly tuned in dewar

– HTSC-filters (Uni Wuppertal);Electr. Tuned by ferro elektric – magnetic material

Piezo electric tuning

Folie 12

Bonn, 30. March 2001RFI Mitigation Workshop12

Example 2: 21cm Receiver

Realized filter bank after the LNAFolie 13

Bonn, 30. March 2001RFI Mitigation Workshop13

Example 2: 21cm Receiver

Planned implementation of High Temperature Superconducting Filters. The filtersare realized.Folie 14

Bonn, 30. March 2001RFI Mitigation Workshop14

1st HTSC Filter: Notch at low end

Folie 15

Bonn, 30. March 2001RFI Mitigation Workshop15

1st HTSC Filter:

Folie 16

Bonn, 30. March 2001RFI Mitigation Workshop16

Example 3: 5cm Receiver

Folie 17

Bonn, 30. March 2001RFI Mitigation Workshop17

Corrugated bandpass filter

Folie 18

Bonn, 30. March 2001RFI Mitigation Workshop18

Corrugated bandpass filter

Fcenter=6.2GHz, RBW=21%; simulation results:

Folie 19

Bonn, 30. March 2001RFI Mitigation Workshop19

CMT + Bandpass integrated

Currently under developmentFolie 20

Bonn, 30. March 2001RFI Mitigation Workshop20

What will be realistic?

In the dewar:– low frequencies > 3 GHz:

1. (tuneable) HTSC filters

– medium frequencies :1. (tunable) waveguide filters

– high frequencies > 30 GHz: fixed waveguide filters

At room temperature:– filters of any kind