Depth of formation of lines in the solar atmosphere.
| Autor: | Achmad, L. |
|---|---|
| Zdroj: | Solar Physics; Apr1992, Vol. 138 Issue 2, p411-414, 4p |
| Abstrakt: | A simple and reliable method has been established for the definition of the depth of formation of lines in a stellar atmosphere. It is based on the determination of the level of emission of the reemitted line radiation. The new definition, which is applied in this paper to the solar case, does not suffer from the ambiguities of previously derived expressions. We apply this method to two artificial weak Oxygen I lines as examples. [ABSTRACT FROM AUTHOR] |
| Databáze: | Complementary Index |
| Externí odkaz: |
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