... During this flaring state there was an extended period (over 21 days) of quenched radio emission (low hard X-ray/high soft X-ray state) which was followed by two major radio flares (13.5 and 17 Jy). ...
... 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 ...
... The flare of 1 Feb was also detected with the Nob eyama 45m and NMA telescop es (Tsub oi et al. 2006), and for the first time a flat radio sp ectrum of the flaring event from Cyg X-3 was directly measured in the quasi-simultaneous observations from 2 to ...
... 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). ...
... The letters about a new expected flare from Guy Pooley (MRAO): . ... Cyg X-3 has finally flared at 15 GHz! ... The light curve of the flare begining at 15 GHz (Rile+RATAN+VLA) . ...
... 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. ...