Please use this identifier to cite or link to this item:
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
ISSN: 82-990556-0-1
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Possible amount of magnetic flux reconnected through quiescent58.28 kBAdobe PDFView/Open

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.