Abstract An intensity time-profile of the hard X-ray emission in two cores of a small impulsive solar flare is analyzed. The emission in the cores proved to evolve in the opposite phases. The phases of growth and decay are also shown to be modulated by the slower oscillatory variations. It is suggested that acceleration processes may be oscillating and a collapsing acceleration process may occur above and below the photosphere.
Solar Flare Peculiarities: A Hypothesis for a New Phenomenological Model
Cosmic Research ; 38 , 6
2000
Article (Journal)
English
BKL: | 55.60 Raumfahrttechnik / 39.00 Astronomie: Allgemeines / 50.93 Weltraumforschung | |
Local classification TIB: | 770/3520/8000 |
Solar Flare Peculiarities: A Hypothesis for a New Phenomenological Model
Springer Verlag | 2000
|NTRS | 1986
|NTIS | 1965
|Solar Flare Patrol and Prediction
NTIS | 1967
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