dc.contributor.author |
Dwivedi, B. N |
|
dc.date.accessioned |
2005-01-08T05:45:03Z |
|
dc.date.available |
2005-01-08T05:45:03Z |
|
dc.date.issued |
1988 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 99-110 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/190 |
|
dc.description.abstract |
The spectroscopic techniques in the X- and EUV region to determine electron density and temperature of solar plasma have been presented. The line intensity ratios as a diagnostic probe of solar plasma from berrylium, boron, nitrogen and oxygen - like ions have been discussed with a detailed investigation of carbon-like ions. Absolute line fluxes from these ions at earth distance have also been discussed. |
en |
dc.format.extent |
391098 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
|
dc.publisher |
Indian Institute of Astrophysics, Bangalore |
en |
dc.subject |
Solar plasma |
en |
dc.subject |
Emission lines |
en |
dc.subject |
Spectral formation |
en |
dc.title |
Diagnostics of solar plasma using emission lines |
en |
dc.type |
Article |
en |