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Hidden Manifestations of Inverse Polarity in Filaments

Published online by Cambridge University Press:  12 April 2016

Boris P. Filippov*
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences, Troitsk, Moscow Region, 142092, Russia

Abstract

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Some aspects of inverse polarity of transverse magnetic fields in filaments are presented following from their fine structure and structure of the chromosphere underneath.

Type
Filaments and Their Environment
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Filippov, B.P. 1995, A&A, 303, 242 Google Scholar
Martin, S.F., Bilimoria, R., and Tracadas, P.W. 1994, in Solar Surface Magnetism, (eds.) Rutten, R.J. and Schrijver, C.J., New York: Springer-Verlag, p. 303 Google Scholar
Rust, D.M. and Kumar, A. 1994, Solar Phys., 155, 69 Google Scholar
Valniček, B., Godoli, G., and Mazzucconi, F. 1968, in Annals of the IQSY, Stickland, A.C., Cambridge, MA: The M.I.T. Press, p. 113 Google Scholar
Webb, D.F. et al. 1994, Solar Phys., 153, 73 Google Scholar