Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/4808
Title: | Possible amount of magnetic flux reconnected through quiescent prominences outside the active regions |
Authors: | Gokhale, M. H Sivaraman, K. R |
Keywords: | Magnetic Flux Solar Magnetic Field Solar Prominences Filaments Photosphere Sunspot Cycle |
Issue Date: | 1979 |
Publisher: | Institute of Theoretical Astrophysics |
Citation: | Jensen, E., Maltby, P and Orrall, F Q. eds., Proceedings of the International Astronomical Union Colloquium No.44 OSLO August 14 - 18, 1978., pp. 189 - 192 |
Series/Report no.: | International Astronomical Union Colloquium; No. 44 |
URI: | http://hdl.handle.net/2248/4808 |
ISSN: | 82-990556-0-1 |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Possible amount of magnetic flux reconnected through quiescent | 58.28 kB | Adobe PDF | ![]() View/Open |
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