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Coronal Structure and Solar Wind

Published online by Cambridge University Press:  14 August 2015

J. N. Tandon
J. N. Tandon*
Affiliation:
Department of Physics & Astrophysics University of Delhi Delhi-110007, India

Abstract

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Recent observations of large scale coronal structures and solar wind have been studied. The intercorrelation of the two have been qualitatively explained through the focussing of solar-ion streams taking account of the local and general solar magnetic fields. This explains the association of coronal holes with weak, diverging open magnetic field lines and envisages the transfer of hydromagnetic wave energy from nearby active centers to account for the enhanced outflow of solar wind associated with coronal holes.

Type
Part I. The Life History of Coronal Structures and Fields
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 73 - 78
Copyright
Copyright © Reidel 1980 

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