Title of article :
Energy release in the 00:18 UT solar flare on April 22, 1994 Original Research Article
Author/Authors :
G.E. Kocharov، نويسنده , , Yu.E. Charikov، نويسنده , , V.P. Lazutkov، نويسنده , , G.A. Matveev، نويسنده , , Yu.N. Nitsora، نويسنده , , M.I. Savchenko، نويسنده , , D.V. Skorodumov، نويسنده ,
Issue Information :
دوهفته نامه با شماره پیاپی سال 2000
Abstract :
We discuss the energy release process in a solar flare. The onset of this flare in soft X-rays was detected at 00:18 UT on April 22nd, 1994, by the IRIS X-ray spectrometer, which was a component of the scientific payload in the international complex research project on solar-terrestrial phenomena on board the CORONAS-I automatic orbital station. An analysis of energy spectra and time profiles of soft X-ray radiation indicates that no usual expansion of flaring volume occurred at the decay of this flare. On the contrary, thermal insulation of the hot plasma could be in effect.
Journal title :
Advances in Space Research
Journal title :
Advances in Space Research