๐”– Bobbio Scriptorium
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The structure of the solar flare stream magnetic field

โœ Scribed by M. I. Pudovkin; S. A. Zaitseva; I. P. Oleferenko; A. D. Chertkov


Publisher
Springer
Year
1977
Tongue
English
Weight
496 KB
Volume
54
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES


Dependence of the flare stream velocity
โœ M. I. Pudovkin; S. A. Zaitseva; S. P. Puchenkina ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› Springer ๐ŸŒ English โš– 429 KB

The main parameters of a flare stream -its velocity, magnetic field intensity, plasma density, and temperature -are shown to depend on the mutual orientation of magnetic fields in the main body of the stream and within its compressed solar wind region. In particular, the plasma velocity and frozen-i

The role of photospheric magnetic field
โœ M. K. Das Gupta; T. K. Das; S. K. Sarkar ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 157 KB

A statistical investigation has been made about the flare-process in relation to the photospheric magnetic field and configuration. It is understood from the analysis that the flare energy bears a linear relationship with the rate of change of flux of the longitudinal component of photospheric magne