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The Solar Corona

Published online by Cambridge University Press:  30 March 2016

Claudio Chiuderi
Claudio Chiuderi*
Affiliation:
Istituto di Astronomia, Università di Firenze (Italy)

Abstract

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Recent observations from space have shown that the solar corona is spatially a very structured medium and temporally a very dynamic one. The consequent changes in the current theoretical ideas about coronal physics are reviewed. The role of the magnetic fields in shaping and heating the coronal structures is especially underlined.

Type
Joint Discussion
Information
Highlights of Astronomy , Volume 5: Highlights of Astronomy. As presented at the XVIIth General Assembly of the IAU, 1979 , 1980 , pp. 335 - 341
Copyright
Copyright © Cambridge University Press 1980

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