Hostname: page-component-77c89778f8-5wvtr Total loading time: 0 Render date: 2024-07-20T08:16:28.387Z Has data issue: false hasContentIssue false
  • English
  • Français

Nonstationary Electric Drifts in the Solar Atmosphere

Published online by Cambridge University Press:  12 April 2016

I.S. Veselovsky
I.S. Veselovsky*
Affiliation:
Institute of Nuclear Physics, Moscow State University

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Induced electric fields and nonstationary drift motions are considered. Nonstationary electric drifts may be important in erupting prominences, rising and shrinking coronal loops, and other phenomena in the solar atmosphere. Theoretical limitations are indicated for the concept of dominant plasma motions along magnetic field lines.

Type
Filaments and Their Environment
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 123 - 126
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Cowling, T.G. 1953, in The Sun Kuiper, G.P. (ed.), The University of Chicago Press, Chicago, p. 532 Google Scholar
Cowling, T.G. 1957, Magnetohydrodynamics, Interscience: N.Y Google Scholar
Gorbachev, V.S. and Kellner, S.R. 1988, Sov. Phys. JETP, 94, 89 Google Scholar
Filippov, B.P. 1996, A&A, 313, 277 Google Scholar
Illiling, R.M.E. and Hundhausen, A.J. 1986, J. Geophys. Res., 91, 10951 Google Scholar
Landau, L.D. and Lifshits, E.M. 1982, Electrodynamics of Continuous Media, Nauka: Moscow (in Russian) Google Scholar
Syrovatskii, S.I. 1969, Astrophys. Space Sci., 4, 240 CrossRefGoogle Scholar
Tandberg-Hanssen, E. 1974, Solar Prominences, D. Reidel: Dordrecht, Holland Google Scholar
Veselovsky, I.S. 1991, Solnechnye Dannye, 11, 89 (in Russian)Google Scholar