OVSA-LWA Spectroscopy AI Summary for 2026/04/12

Section: Summary
The solar radio activity on 2026-04-12 was very low. Solar tracking began at approximately 13:25 UTC, marked by a sharp transition from the non-tracking state in the first spectrogram. For the remainder of the day, the background flux levels were stable at around 1 sfu.

A few minor transient features were observed, most notably two weak Type III-like bursts occurring at 15:49 UTC (Image 6) and 18:12 UTC (Image 10). However, due to the extremely narrow range of the color scales used in these spectrograms (with labels such as $10^0$ and $2 \times 10^0$), these features are estimated to have peak fluxes well below 5 sfu. No significant radio bursts exceeding the 10 sfu threshold were detected during the observation period, and the day is classified as quiet.

Section: Events
Event # | Begin UT | Peak UT | End UT | Freq Range | Peak Flux | Type | Spectrogram URL
No events with flux above 10 sfu were detected.