OVSA-LWA Spectroscopy AI Summary for 2026/04/10

Section: Summary
The solar radio activity on 2026-04-10 was extremely quiet. Solar tracking by the OVRO-LWA array began at approximately 13:25 UTC, as indicated by the sharp transition in the first spectrogram. Throughout the remainder of the observing day, the background flux density remained consistently low, typically fluctuating around or below the 1 sfu level. No solar radio bursts were detected above the 10 sfu threshold.

The spectrograms show standard narrow-band radio frequency interference (RFI) and some minor instrumental artifacts. A large block of data in the final spectrogram (Image 9) between 17:16 UTC and 17:30 UTC appears to be a result of instrumental saturation or a calibration issue rather than solar activity. The Stokes V/I panels confirm the lack of any significant polarized solar emission during the observed period.

Section: Events
Event # | Begin UT | Peak UT | End UT | Freq Range | Peak Flux | Type | Spectrogram URL
No events were detected.