dc.contributor.author |
Raju, P. K |
|
dc.contributor.author |
Dwivedi, B. N |
|
dc.date.accessioned |
2008-12-16T14:19:33Z |
|
dc.date.available |
2008-12-16T14:19:33Z |
|
dc.date.issued |
1978-12 |
|
dc.identifier.citation |
Solar Physics, Vol. 60, No. 2, pp. 269 - 277 |
en |
dc.identifier.issn |
0038-0938 (Print) 1573-093X (Online) |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4073 |
|
dc.description |
Open Access |
|
dc.description.abstract |
Assuming steady state conditions, the occupation of 9 levels of oxygen-like ions: Ne iii, Mg v, Si vii, S ix, and Ar xi have been computed as a function of electron density and temperature. The following physical processes have been considered: collisional excitations and spontaneous radiative de-excitations for permitted and intercombination transitions; collisional excitations and de-excitations, photo-excitations and spontaneous radiative transitions among the five levels of the ground term. This study indicates that line intensity ratios for oxygen-like ions can be used as a diagnostic in the determination of these two parameters of the solar plasma. |
en |
dc.language.iso |
en |
en |
dc.publisher |
D.Reideal Publishing Co., |
en |
dc.relation.uri |
http://dx.doi.org/10.1007/BF00156527 |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1978SoPh...60..269R |
en |
dc.rights |
©D.Reideal Publishing Co., |
|
dc.subject |
Solar Emission |
en |
dc.subject |
Electron Density |
|
dc.subject |
Atomic Data |
|
dc.title |
Density dependence of solar emission lines of oxygen-like ions |
en |
dc.type |
Article |
en |