Hi everyone,
I am currently working on an RFI-detection project using waterfall spectrograms from UOBGS and comparing them with observations from SatNOGS Station 91 – M0EYT / 2E0NOG.
The satellite I am analysing is ROBUSTA-3A (NORAD 60243) around 436.750 MHz.
I would really appreciate some guidance from the SatNOGS community on the most scientifically appropriate way to perform this comparison.
For the UOBGS observations, I have the original numerical waterfall recording files in .dat format. From these I can recover the time-frequency waterfall matrix and perform numerical processing.
For the corresponding SatNOGS Station 91 observations, however, what I currently have available is mainly:
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observation metadata,
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waterfall PNG images,
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audio where available,
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observation timing and transmitter information.
My main question is:
How would you recommend comparing the two stations’ waterfalls to investigate whether an unusual spectral feature is likely to be RFI?
For example, if an anomalous feature appears in the UOBGS waterfall, I would like to investigate whether a corresponding feature is also visible at Station 91 at the same absolute UTC time and corresponding RF frequency.
At the moment I am considering:
UOBGS .dat numerical waterfall → anomaly/RFI-candidate detection → UTC/frequency registration → comparison with the Station 91 waterfall.
However, because the Station 91 product available to me is a rendered PNG rather than the same type of numerical waterfall data, I am unsure what comparison method would be considered scientifically defensible.
In particular, I would really appreciate advice on:
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How best to align the two observations in UTC and RF frequency, considering that each station experiences a different Doppler trajectory.
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Whether comparing spectral morphology/features between a numerical
.datwaterfall and a SatNOGS PNG is reasonable, and what metrics or methods would be recommended. -
How SatNOGS users normally distinguish a genuine RFI feature from receiver artefacts, satellite signal structure, noise, or processing artefacts in waterfalls.
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Whether the absence of a feature at Station 91 can provide meaningful evidence that an anomaly observed at UOBGS is local, or whether receiver/antenna/sensitivity differences make that conclusion unsafe.
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Whether the original numerical waterfall data used to generate the Station 91 PNGs may exist somewhere, for example as a
.dat, HDF5 waterfall, or another numerical product.
If numerical Station 91 waterfall data are available, that would potentially allow a much more direct time-frequency comparison with my UOBGS .dat recordings.
I already have several same-pass ROBUSTA-3A observations from Station 91 and can provide the exact observation IDs, UTC dates and times if that would help.
Any advice on how SatNOGS operators/researchers would approach this comparison would be greatly appreciated.
Thank you!
