... Region 9373 (S07W43) produced several small C-class flares. One flare at 18/0850 UTC was an C3/1f . ... One flare at 18/0850 UTC was an C3/1f . with an associated Type II radio sweep. ...
... Flare Origin - critical analysis" Lev Pusti'lnik We analyze current approach to ... flare energy release in final .flare. state of current-magnetic system and show that ...
... After this flare, there was a sharp decrease in the radio intensity on May 29--31, to 15--20 mJy at 4--11 GHz, 10--12 days before a powerful flare on June 12 (~4 Jy). ...
... In comparison, a large flare lasts for only a few minutes, but the preliminary stage of the flare - the increase of the complexity of the magnetic structure, the emergence of new magnetic tubes - takes up to three days. ...
... Solar flare activity is produced by the processes of accumulation and release of ... formed over the spots, the reconnection of which leads to the generation of a flare ...
... S., Bogod V., Detection of the long-term microwave "darkening" before the July 14, 2000 flare //Solar Physics, 212/1, pp ... of Microwave emission from Active Regions Generating Intense Solar Flares // Astronomy Letters, 2003/4, pp.263-273 ...