dc.contributor.author |
Dwivedi, B. N |
|
dc.contributor.author |
Raju, P. K |
|
dc.date.accessioned |
2009-09-10T10:09:43Z |
|
dc.date.available |
2009-09-10T10:09:43Z |
|
dc.date.issued |
1988 |
|
dc.identifier.citation |
Advances in Space Research, Vol. 8, No. 11, pp. 179 - 183 |
en |
dc.identifier.issn |
0273-1177 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4805 |
|
dc.description.abstract |
Steady state level population of 13 levels of nitrogen-like ions; Ne IV, Mg VI, Si VIII, and S X have been computed as a function of electron density and temperature. We have accounted for collisional and spontaneous radiative processes. Photo-excitations among the ground term levels have also been considered. Using the computed level populations line intensities have been obtained as a function of electron density and temperature. This study indicates that line intensity ratios for nitrogen-like ions can be used as a density monitor of the solar plasma. Absolute line fluxes from these ions at earth distance have been computed and compared with values obtained using various satellite and rocket measurements |
en |
dc.language.iso |
en |
en |
dc.publisher |
Elsevier |
en |
dc.relation.uri |
http://dx.doi.org/10.1016/0273-1177(88)90316-X |
en |
dc.rights |
© Elsevier |
en |
dc.subject |
Density Diagnostics |
en |
dc.subject |
Solar Emission Lines |
en |
dc.subject |
Nitrogen-Like Ions |
en |
dc.title |
Density diagnostics of solar emission lines from nitrogen-like ions |
en |
dc.type |
Article |
en |