[evlatests] High-Speed RFI!
Bryan Butler
bbutler at nrao.edu
Mon Oct 3 18:41:55 EDT 2016
if he was talking about SMAP, that's L-band. i don't know of an
orbiting NASA satellite doing radar at C-band. not that i know
everything that's up there! there are two ESA C-band SARs - Sentinel-1
and Sentinel-2 that might fit the bill, but they don't go over every day...
-bryan
Barry Clark wrote on 10/3/16 16:22 :
> One of the tour participants at the openhouse Saturday said NASA
> has a downlooking radar satellite that probably passes, rather
> rapidly, over the VLA about noon or a little later every day.
>
> On 10/03/2016 03:38 PM, Rick Perley wrote:
>> In calibrating astronomical data, mostly taken last year, a
>> remarkable type of RFI has been seen.
>>
>> Observations were made in all four configurations at C-band. Over
>> one year elapsed between the first and last of these observations.
>>
>> The effect was noted in the gains, starting with the
>> D-configuration data. In this configuration, it was noted that all 16
>> spectral windows had a reduced amplitude, for all antennas, both
>> polarizations, by about a factor of two. The effect lasted 30 seconds,
>> after which all gains were again normal. Only one event was seen.
>>
>> Investigation (via 'SPFLG') showed that the cause was a strong RFI
>> signal, located within SPW3 (spanning 4232 -- 4360 MHz). The data in
>> this SPW had very large and random values, presumably due to overflow in
>> the accumulators. All other SPWs retained their coherency, but the
>> amplitudes were reduced. Phases were unaffected.
>> The signal was strong enough that the entire 2 GHz bandpass was
>> compressed enough to lower the gains by a factor of up to two.
>> There were two C-band IF tunings in this experiment -- the other
>> one (6 -- 8 GHz) showed no effect, indicating the the compression is in
>> the IFs, not in the receiver.
>>
>> But much more interesting (to me, at least) is that the data from
>> the C, B, and A configurations also showed similar compression. But the
>> much larger spatial scale of these configurations clearly show that the
>> range of the RFI effect is localized, and moving at high speed.
>>
>> The evidence is clearest for the A configuration. There were four
>> 'events' during this run (which was taken in July 2015). For all four,
>> the effect was localized to a a subset of the array. For all four, only
>> the antennas on one or two arms were affected. In all cases, the
>> strength of the compression varied along the antennas of the arm
>> affected -- usually with the end-most antenna the most strongly affected.
>> The timing of the 'events' gives us a pretty good estimate of the
>> velocity. The peak saturation for one of these four events showed a 30
>> second lag between the end antenna of the east arm and a middle antenna
>> of the north arm (and with the peak progressively later for antennas
>> along the east arm). That translates to ~ 2000 mph!
>>
>> Might this be some sort of satellite imaging radar? It's clearly
>> highly focused, and moving quite quickly.
>>
>>
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