The flare triggers predominantly the surface LPDAs in stations 12 and 23. In station 12 it is evident, that the flare has increased the trigger threshold in the lower rate of surface triggers after the flare compared to before. Station 21 is closest to Summit Camp, and is more exposed to anthropogenic noise. The higher threshold of the surface component thus leads to deep triggers during the flare.
Only the first of the brighter type III's leads to a significant number of triggered events. In the spectrograms however it is followed by a similarly bright partner. The couple is accompanied by two smaller 'children'.
While the spectrograms reveal multiple discernible type III flares spread over serveral minutes, only one of them i able to consistently surpass the trigger threshold in all stations.
The bright type III flare led to high trigger rates in all stations. The subsequeny type II is drifting away from the solar photosphere to lower frequencies over ~15 minutes and is only visible in the surface LPDA spectra, but does not trigger the RNO-G stations.
An isolated burst of events seen in stations 11 and 21. Unfortunately the other stations were not taking data for this flare.
This isolated flare is visible in the spectrograms beyond 350 MHz and coincidently triggers all stations.
While a less strong additional type III flare is still visible in the surface spectrograms 1.5 minutes later, only the main flaring activity surpasses the trigger threshold in the RNO-G stations.
A distinct narrowband feature inside the flare is able to trigger the RNO-G stations. In the spectrograms, the harmonics for the type II are visible, towards the end of the window, the flare shows up in the low-frequency Callisto instrument.
A twin pair of type III bursts occuring within 3 minutes. Just as in real live, one twin might be more impulsive than the other, and trigger more stations.
On July 11, 2022, broadband emission was also observed over many hours in various Callisto stations. The trigger rates and spectra show fluctuation over an extended period of time. Note that the trigger rate excess here occured during night, where no human activity near the stations is expected.
The series of individual type III flares is spread over several minutes and allows 'tracking' of the Sun on the sky.
Strong type III activity with at least three individual bursts able to trigger all RNO-G stations. Narrowband background source is visible ~2 minutes before the flare.
This type III is strong and extended enough to trigger stations for over a minute. Note that the time offset at that time is a known issue to HUMAIN.
Two strong type III's triggering all stations, followed by another, weaker, type III a few minutes later.