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Étude critique d'un champ ‘current-free’ dans l'atmosphère solaire∗

Published online by Cambridge University Press:  14 August 2015

J. Rayrole  and
M. Semel
J. Rayrole
Affiliation:
Observatoire de Meudon (S.& O.), France
M. Semel
Affiliation:
Observatoire de Meudon (S.& O.), France

Abstract

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To test the validity of the assumption of a ‘current-free’ magnetic field in the atmosphere above sunspots, we measured all three parameters of the magnetic field in an active region and compared it with the calculated current-free field according to the solution proposed by Schmidt. We found important differences between the calculated and the measured field.

We refer to an earlier paper where the objections to the ‘current-free field’ were that the calculated field has too simple a configuration to account for the fine structure observed in Hα and other solar observations.

Type
Part II: Theoretical Aspects
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 134 - 141
Copyright
Copyright © Reidel 1968 

References

Références

Godovnikov, N.V., Smirnova, E.P. (1965) Izv. krym. astrofiz. Obs., 33, 86.Google Scholar
Oster, L. (1964) Ann. Astrophys., 27, 14.Google Scholar
Rayrole, J. (1967) Ann. Astrophys., 30, 257.Google Scholar
Schatzman, E. (1961) Ann. Astrophys., 24, 251.Google Scholar
Schmidt, H.U. (1964) NASA Solar Flare Symposium, Nasa SP-50, 107.Google Scholar
Semel, M. (1967) Ann. Astrophys., 30, 513.Google Scholar
Tandberg-Hanssen, E. (1967) Solar Phys., 2, 98.Google Scholar