OVSA-LWA Spectroscopy AI Summary for 2026/04/03

Section: Summary
Solar radio activity on 2026-04-03 was characterized by low to moderate levels of Type III radio burst activity. Following the start of solar tracking at approximately 13:40 UTC, numerous small groups of weak Type III bursts were observed intermittently throughout the day. While many of these features were visible, most remained below the 10 sfu threshold.

The most significant activity was a group of Type III bursts occurring between 19:28 and 19:34 UTC, with peak emission around 19:31 UTC reaching approximately 25 sfu. Another notable burst was observed later at 01:18 UTC on April 4th, reaching an estimated peak flux of 15 sfu. No strong bursts exceeding 100 sfu were detected, and there were no observations of long-lived noise storms or Type II and Type IV bursts during this period.

Section: Events
Event # | Begin UT | Peak UT | End UT | Freq Range | Peak Flux | Type | Spectrogram URL
1 | 1928 | 1931 | 1934 | 20-85 | 25 sfu | Type III burst group | https://ovsa.njit.edu/lwa-data/qlook_spectra/2026/04/03/20260403-193740-lwa_beam.png
2 | 0117 | 0118 | 0121 | 20-85 | 15 sfu | Type III burst | https://ovsa.njit.edu/lwa-data/qlook_spectra/2026/04/04/20260404-013203-lwa_beam.png