... 16b. Carrington's Flare . ... And for scientists: a contemporary article on Carrington's flare, The extreme magnetic storm of 1-2 September 1859 by Bruce T ...
... main specific features of large-scale reconnection as the physical phenomenon responsible for accumulation of energy before a large flare and for a fast release of this energy during a flare, including acceleration of electrons and ions to high energies ...
... The model can readily explain the minute-scale TeV flares on top of longer (typical time-scales of days) gamma-ray variability as observed from the blazer PKS2155-304 and day-scale TeV flares from M87. ...
... 0.1 to 0.8 nm band as follows: Class W/m*2 Ergs/cm*2/s B I < 10E-6 I < 10E-3 C 10E-6 <= I < 10E-5 10E-3 <= I < 10E-2 M 10E-5 <= I < 10E-4 10E-2 <= I < 10E-1 X I >=10E-4 I >=10E-1 ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SOLAR_FLARES/XRAY_FLARES/xray.fmt.rev ...
... CY lindrical GA mma-ray M onitor . SOLAR FLARES . ... with energies up to 300 MeV from the solar flare on 26.03.1991 registered by the ... Schematic model of the solar flare. table of contents . previous page . next page . ...
... near the Earth and the solar flare in different electromagnetic wave lengths on 2005 ... in favor of the prolonged and multiple accelerations of protons in solar flares ...