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Empirical Models of Photospheric Flux Tubes

Published online by Cambridge University Press:  08 February 2017

S.K. Solanki
S.K. Solanki*
Affiliation:
Department of Mathematical Sciences, Unversity of St Andrews, St Andrews, KY16 9SS, Scotland

Abstract

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The empirically derived properties of magnetic flux tubes at both ends of the size spectrum, i.e. magnetic elements and sunspots, are reviewed. Emphasis is placed on quantitative results. The following parameters are discussed in greater detail: The strength and structure of the magnetic field, the temperature stratification and the structure of the velocity field.

Type
III. Small-Scale Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 138: Solar Photosphere: Structure, Convection and Magnetic Fields , 1990 , pp. 103 - 120
Copyright
Copyright © Kluwer 1990 

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