|
|||||
|
|
A simplified model solar atmosphere |
|
| Authors: | D L Lambert |
| Institution: | (1) Dept. of Astrophysics, University Observatory, Oxford |
| Abstract: | A simplified representation of the temperature distribution in the solar photosphere is proposed:  (
0) =
0 -
1 log
0. An expression is derived for the emergent continuous spectrum from the simple model. The limitations and applications of the simple model are discussed. |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ | |