| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9599124 | Journal of Quantitative Spectroscopy and Radiative Transfer | 2005 | 5 Pages |
Abstract
There are some solar prominence fine structures which are not observable. Thus, we need to use theoretical methods to study their geometric and physical properties. It is believed that observed intensities, and their fluctuations are related to such fine structures in the line of sight. Regarding the fact that analysis of intensity and its fluctuations necessitates the knowledge of the dependence of scattering albedo relative to optical depth, the present study is an attempt to determine scattering Albedo functions which are more probable to reality from the astrophysics' perspective.
Related Topics
Physical Sciences and Engineering
Chemistry
Spectroscopy
Authors
A. Adjabshirizadeh, H. Ebadi,