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The role of photospheric magnetic field in the development of solar flares

โœ Scribed by M. K. Das Gupta; T. K. Das; S. K. Sarkar

Publisher
Springer
Year
1981
Tongue
English
Weight
157 KB
Volume
69
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

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 magnetic field.

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The amount of energy released during a solar flare and the relatively short timescale in which all the flare associated events occur lead to the conclusion that a solar flare is a magnetohydrodynamic instability taking place in a strongly turbulent plasma. The main effect of the plasma turbulence i