Abstract Radio bursts in the frequency range 100–1500 kHz and fluxes of energetic electrons with energies of 20–450 keV recorded onboard the Interball-1 satellite during prominent chromospheric flares on the Sun are studied. The time of propagation of the electrons to the Earth is estimated using the method of comparison of the moments of the beginning of radio emission generation during the explosive phase of the flare and the arrival of the accelerated electrons to the Earth.
Hectometer radio bursts and energetic electrons during solar flares according to observations onboard the Interball-1 satellite
Cosmic Research ; 44 , 3
2006
Aufsatz (Zeitschrift)
Englisch
BKL: | 55.60 Raumfahrttechnik / 39.00 Astronomie: Allgemeines / 50.93 Weltraumforschung | |
Lokalklassifikation TIB: | 770/3520/8000 |
Investigation of Long-Wave Radio Bursts from Interball-1 Satellite Observations
Springer Verlag | 2002
|Investigation of Long-Wave Radio Bursts from Interball-1 Satellite Observations
Online Contents | 2002
|A Study of Long-Wave Radio Bursts Observed in 2000 onboard the INTERBALL-1 Satellite
Online Contents | 2003
|Observations of the auroral hectometric radio emission onboard the INTERBALL-1 satellite
Online Contents | 2007
|