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Theories of Small-Scale Magnetic Fields
Published online by Cambridge University Press: 14 August 2015
Abstract
This review is concerned with the origin of the fine structure of the fields and their relationship to the heating of the solar chromosphere and corona, the structure of prominences and the production of energetic particles in solar flares. The dynamics of sunspot formation, and the large-scale structure of individual sunspots have not been dealt with, although the evolution of AR fields has been considered insofar as it affects the flare problem.
- Type
- Part V: Theories of Small Scale Magnetic Fields
- Information
- Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 457 - 474
- Copyright
- Copyright © Reidel 1971
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