Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/4291
Title: | Can coronal magnetic structures be quasi-static? |
Authors: | Venkatakrishnan, P |
Keywords: | Coronal Magnetic Structures Quasi-Static |
Issue Date: | 1994 |
Publisher: | Astronomical Society of the Pacific |
Citation: | K. S. Balasubramaniam and George W. Simon., eds., Solar active region evolution: comparing models with observations. Astronomical Society of the Pacific Conference Series, Vol. 68, Proceedings of the 14th International Summer Workshop, National Solar Observatory / Sacramento Peak, Sunspot, New Mexico, USA, 30 August - 3 September 1993, pp. 409 - 410 |
Series/Report no.: | Astronomical Society of the Pacific Conference Series, Vol. 68 |
URI: | http://hdl.handle.net/2248/4291 |
Appears in Collections: | IIAP Publications |
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Can coronal magnetic structures be quasi-static? | 175.36 kB | Adobe PDF | View/Open |
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