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
Pages
4
From page
1817
To page
1820
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
Serial Year
2000
Journal title
Advances in Space Research
Record number
1126840
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