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Particles and Energy Transport in the Solar Atmosphere during Solar Flares
Published online by Cambridge University Press: 27 September 2017
Abstract
The proposed model of particles transport in the solar atmosphere during flares consists in a low density plasmoid originating deep in the atmosphere and rising under magnetic and buoyancy forces. Confined particles are selectively released during the ascent and their interaction with the solar atmosphere produces X and γ bremsstrahlung. The characteristics of high energy particles released in the interplanetary medium are found to agree with observations.
- Type
- Session III: Theory
- Information
- International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 321 - 324
- Copyright
- Copyright © Kluwer 1989