dc.contributor.author |
Dwivedi, B. N |
|
dc.date.accessioned |
2005-02-10T13:51:45Z |
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dc.date.available |
2005-02-10T13:51:45Z |
|
dc.date.issued |
1986 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 38-48 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/359 |
|
dc.description.abstract |
A general discussion of solar flares with emphasis on two-ribbon flares is given. The basic differences between compact (simple-loop) and two-ribbon flares have also been pointed. Skylab observations have been presented to show that the hot loops are seen first in X-rays, later in extreme ultraviolet lines and, after an appropriate cooling time, in H-aplha as the loop prominence systems. Particle acceleration during a long-enduring reconnection process in two-ribbon flares have been discussed. |
en |
dc.format.extent |
442589 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
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dc.publisher |
Indian Institute of Astrophysics, Bangalore |
en |
dc.subject |
solar flares |
en |
dc.subject |
skylab observations |
en |
dc.title |
Our Present Understanding of Solar Flares |
en |
dc.type |
Article |
en |