OVSA-LWA Spectroscopy AI Summary for 2026/04/05

Section: Summary
The solar radio tracking for the OVRO-LWA on April 5, 2026, began during the 13:00 UTC hour. For most of the observation period, the day was quiet, with solar radio activity remaining at very low levels. The spectrograms show a primarily quiescent Sun, punctuated only by a few instances of weak, short-lived Type III radio activity.

The only burst event identified with a peak flux exceeding the 10 sfu threshold occurred between 23:30 and 23:33 UTC. This event consisted of a small group of Type III bursts with an estimated peak flux of approximately 15 sfu. Other marginal features and very weak bursts were visible at various times (notably around 18:17, 20:08, and 21:33 UTC), but their intensities remained below the detection threshold for significant events. No strong bursts (>100 sfu), Type II, or Type IV events were recorded during the day.

Section: Events
Event # | Begin UT | Peak UT | End UT | Freq Range | Peak Flux | Type | Spectrogram URL
1 | 2330 | 2331 | 2333 | 30-85 | 15 sfu | Type III burst group | https://ovsa.njit.edu/lwa-data/qlook_spectra/2026/04/05/20260405-234018-lwa_beam.png