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On the magnetic-field structure around filaments

Published online by Cambridge University Press:  14 August 2015

B. A. Ioshpa
B. A. Ioshpa*
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere and Radio-Wave Propagation of the U.S.S.R. Academy of Sciences, Moscow

Extract

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The results of an investigation of the magnetic-field structure in the chromosphere around filaments are briefly given in this paper. The hypothesis of the existence of a two-field system is suggested: an outer field which has the form of arches and supports the filament against gravity, and an inner one, directed along the filament.

Type
Part III: Optical Structure of an Active Region
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 261 - 266
Copyright
Copyright © Reidel 1968 

References

Howard, R., Harvey, J. W. (1964) Astroph. J., 139, 1335.Google Scholar
Ioshpa, B. A. (1967) Soln. Aktivnost, 3.Google Scholar
Ioshpa, B.A., Obridko, V.N. (1966) in Proceedings of the Meeting on Solar Magnetic Fields and High Resolution Spectroscopy, Roma, II, No. 4, p. 161.Google Scholar
Kippenhahn, R., Schlüter, A. (1957) Z. Astrophys., 43, 36.Google Scholar
Stepanov, W.E. (1959) Izv. Krym. astrofiz. Obs., 20, 52.Google Scholar
Zhulin, I. A., Ioshpa, B. A., Mogilevsky, E.I. (1965) Soln. Aktivnost, 2, 108.Google Scholar