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Particles and Energy Transport in the Solar Atmosphere during Solar Flares

Published online by Cambridge University Press:  27 September 2017

Heristchi D. ,
Raadu M.A. ,
Vial J.-C.  and
Malherbe J.-M.
Heristchi D.
Affiliation:
Observatoire do Paris, Section de Meudon, Dasop, U.A. 326, 92195 Meudon Principal Cedex, France
Raadu M.A.
Affiliation:
Royal Institute of Technology, Department of Plasma Physics, S-100 44 Stockholm, Sweden
Vial J.-C.
Affiliation:
I.A.S/ Laboratoire de Physique Stellaire et Planétaire, B.P. 10, 91371 Verrières-ie-Buisson Cedex, France
Malherbe J.-M.
Affiliation:
Observatoire do Paris, Section de Meudon, Dasop, U.A. 326, 92195 Meudon Principal Cedex, France

Abstract

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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

References

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