dc.contributor.author |
Narain, Udit |
|
dc.contributor.author |
Kumar, Mukul |
|
dc.date.accessioned |
2005-02-11T05:34:05Z |
|
dc.date.available |
2005-02-11T05:34:05Z |
|
dc.date.issued |
1986 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 127-131 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/369 |
|
dc.description.abstract |
In this article the heating of solar corona by magnetic fields, with particular emphasis to the work done by authors has been presented. It is found that the heating of active ragions by twisting of magnetic fields (Tucker, 1973) does not seem feasible in view of very high twisting velocities predicted for the magnetic field. Further the heating by reconnection (Levine, 1974) seems interesting and needs further quantitative investigation. |
en |
dc.format.extent |
139882 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
|
dc.publisher |
Indian Institute of Astrophysics, Bangalore |
en |
dc.subject |
Solra Corona |
en |
dc.subject |
Magnetic Fields |
en |
dc.title |
On Heating of Solar Corona Through Magnetic Fields |
en |
dc.type |
Article |
en |