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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| File | Description | Size | Format | |
|---|---|---|---|---|
| Can coronal magnetic structures be quasi-static? | 175.36 kB | Adobe PDF | ![]() View/Open |
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