After about 34:00 in the 9th press conference of AAS 235, radio astronomer and NRAO's spectrum manager Harvey Liszt talks about Radio Astronomy in a New Era of Radio Communication and says:

This is a new development that we’re going to have to come to grips with. There is a band allocated between 9.2 and 10.4 GHz (this is roughly an order of magnitude lower than you saw for CloutSat) and these are being developed commercially now, and if you look on the right you’ll see ICEYE. ICEYE’s slogan is “Every square meter, Every hour”.

A synthetic aperture radar like this, if pointed at a radio telescope when the telescope is pointed in its direction will burn out the radio astronomy receiver.

As a matter of fact, some of these radars are so strong that even the ground scatter (the albedo of the ground is about 10%) and even the backscatter from radar will burn out a radio astronomy receiver.

One of the radar constellation companies named by Dr Liszt as posing a potential problem is Finland's Iceye.

The firm's CEO, Rafal Modrzewski, said his team took its responsibilities seriously, and that it continued to investigate any potential risks Iceye's technology might pose to the global space community, both in orbit and on the ground.

"Most importantly in this topic, Iceye complies with international regulation regarding our allocated bands," he told BBC News.

"Mitigating any potential or perceived risks to sensors on ground can additionally be done proactively by tracking applicable SAR satellite orbits to avoid clashes with instrumentation, and in the case of Iceye, by also working with us if there are any remaining concerns."

At the recent American Astronomical Society meeting in Hawaii, Dr Harvey Liszt from the US National Radio Astronomy Observatory raised the concern that powerful radar pulses from orbit could damage the radio receivers that scientists employ in their ground observatories.

(Capella's CEO) Payam Banazadeh told me Capella was taking this matter very seriously and was keen to co-ordinate his company's activities with the AAS.

"We have also been in contact with Dr Liszt and are actively working to safeguard their mission when operating our SAR constellation.

"Whether it is observing Earth or deep space, Capella believes in exploration and scientific discovery. We also believe in and support protecting the mission of the radio astronomy community."

1. Do they keep track of known satellites and "avert their eyes" by steering dishes away from expected trajectories?
2. Is this planned during a scheduling phase or during an observation?
3. Would this kind of interruption and movement be detrimental to the quality of data for a long observation?

• Do these sources actually damage the detector or just cause it to saturate and ruin lots of potentially useful data? Sep 16, 2021 at 22:08
• @honeste_vivere it's hard to find sources to cite (still working on it) but I have been told that when a synthetic aperture radar (SAR) satellite sweeps its ground-scanning radar beam over a large dish antenna, it can really burn out the front-end amplifier. And these days there are some serious SAR satellites constantly mapping the Earth.
– uhoh
Sep 16, 2021 at 22:55
• Really? Wow, that's kind of alarming and disappointing... One would think there would be a way to protect them but I assume that would compromise sensitivity? Sep 17, 2021 at 14:42

There are a number of approaches to avoid the impact of radio frequency (RF) emitters in radio astronomy. This interference can impact performance even if it is not at level that is significant to cause damage. In the end they all come down to trade offs between sensitivity and robustness in the presence of interference.

Spectrum Allocation
The first means of protection is simply to avoid observing in at the same frequencies that other systems use to transmit. A number of frequency bands are reserved for radio astronomy use and other systems are to avoid operating in these bands. These allocations can differ by geographical region and between terrestrial and satellite platforms. For the band mentioned in the question, 9.2-10.4 GHz, there is no allocation for radio astronomy, so you would have to deal with whatever interference may be present. (Gory details for the US can be found in FCC Online Table of Frequency Allocations.)

The International Telecommunications Union (ITU) publishes a large number of recommendations related to protecting radio astronomy. These include (not a complete list):

• RA.314, Preferred frequency bands for radio astronomical measurements
• RA.517, Protection of the radio astronomy service from transmitters operating in adjacent bands
• RA.611, Protection of the radio astronomy service from spurious emissions
• RA.769, Protection criteria used for radio astronomical measurements
• RA.1031, Protection of the radio astronomy service in frequency bands shared with active services

Filtering
The next best thing to do is provide RF filtering to reject signals that are outside of the band being studied. These filters introduce loss that results in some desensitization. Current state of the art is probably high temperature superconducting (HTS) filters. The can archive particularly low loss levels, for example less than 0.1 dB in L-band (1.40 - 1.72 GHz).

An example of a radio astronomy receiver incorporating filtering for RF interference rejection can be found in High Performance Receiver for RFI Mitigation in Radio Astronomy: Application at Decameter Wavelengths.

To prevent receiver damage from excessive input signals, particularly in-band, where filtering would be ineffective, an RF power limiter may be employed. One type of limiter, the PIN limiter diode, as described in PIN Limiter Diodes in Receiver Protectors:

The PIN limiter diode can be described as an incident power- controlled, variable resistor. In the case when no large input signal is present, the impedance of the limiter diode is at its maximum, thereby producing minimum insertion loss, typically less than 0.5 dB. The presence of a large input signal temporarily forces the impedance of the diode to a much lower value, producing an impedance mismatch which reflects the majority of the input signal power back towards its source.

For those interested, a receiver architecture incorporating such listing can be found in Electronics Division Internal Report No, 113 3-Element Interferometer 3,7, 11, and 21 cm Receivers. This document describes one of the receivers used at the National Radio Astronomy Observatory at Green Bank, West Virginia. I have reproduced part of one of the block diagrams below highlighting the receiver limiting.

Processing Algorithms
A final approach is to use digital processing algorithms to ignore data that has been subject to radio frequency interference (RFI):