OVSA-LWA Spectroscopy AI Summary for 2026/04/11

Section: Summary
The solar radio activity on April 11, 2026, was characterized by an extremely quiet Sun. The array began tracking the Sun at approximately 14:15 UTC, following the usual early morning non-tracking period. Throughout the observation day, the background flux remained stable at a very low level, typically around 1 sfu across the entire frequency range.

A few marginal and weak features were observed, including a small group of faint Type III bursts between 19:55 and 20:00 UTC (Image 12) and a solitary, weak Type III burst near 23:56 UTC (Image 19). Both of these features were exceptionally faint, with peak fluxes estimated to be less than 2 sfu, significantly below the 10 sfu reporting threshold. No significant solar radio bursts or storms were detected during the day.

Section: Events
No events detected above 10 sfu.