[evlatests] 128-MHz spectral artifacts

[Ken Sowinski]

A reminder that so far this has only been seen at L band so if LO
spurs are the explanation, it could be the L301 rather than the L302.
Band dependence might be investigaed by observing 'mega-masers', or by
setting up a beacon at any convenient frequency.



On Fri, 30 Aug 2024, Paul Demorest via evlatests wrote:

> Hi all,
>
> Thanks to some careful investigation of L-band RFI by Lilia and Pedro, we have found a new (at least to us) type of spectral artifact in EVLA data.  We see low-level, frequency-shifted copies of strong RFI lines at frequencies +/- 128 MHz (and likely +/- 256 MHz as well) away from the real signal.  These signals are about -45 dB in power relative to the real signal, though this ratio is still somewhat uncertain due to the large signal strength and potential non-linearity.  We can see these most easily around 1425 MHz in the clean/protected part of L-band when pointing in specific directions, due to strong satellite RFI around 1550 MHz.
>
> We currently do not think this is a correlator artifact because:
>  - The copies appear at the same sky frequency and amplitude independent of WIDAR subband BW (for 64 and 128 MHz subbands).
>  - They also appear the same when the LO tuning is shifted slightly, thus moving the signal position with the subbands.
>  - There is no change in their amplitude when the WIDAR "F-shift" is disabled.  (Other different artifacts do appear, as expected, when F-shift is turned off)
>
> This behavior appears on all four IFs, and on all baselines.  We might want to quantify the antenna/baseline dependence a bit better, but it does not appear to be limited to one or a few specific antennas.  We don't know if this is a new thing or has always been there.  It does require a very strong input signal to become noticeable.
>
> Some plots are attached to show how this looks.  These show "scalar-averaged" visibility data versus frequency from some of our recent experiments, for a variety of correlator setups and tunings.
>
> One explanation that we think fits the data is if an LO has low-level spurs at N*128 MHz away from the main tone.  This seems vaguely plausible to me since the L302's use a 128-MHz comb as part of their signal generation.  Of course others on this list know much more about the internals than I do.  It would be interesting to know if this sort of thing has been measured for the L302 output.  If not maybe someone could run some spectrum analyzer tests?  I'll put in a Jira ticket shortly for those who would rather track this there.
>
> Other suggestions are welcome of course!
>
> Cheers,
> Paul