Análisis de anchos equivalentes de líneas del espectro solar
In order to detect possible systematic erros, a quality analysis of Moore, Minnaert and Houtgast (MMH) equivalent widths for the solar liens is undertaken. The results do not show significant dependences on the equivalent width or the wavelength of the line. A trend for the internal dispersion of MM...
Guardado en:
| Autor principal: | |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1987
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/132283 |
| Aporte de: |
| Sumario: | In order to detect possible systematic erros, a quality analysis of Moore, Minnaert and Houtgast (MMH) equivalent widths for the solar liens is undertaken. The results do not show significant dependences on the equivalent width or the wavelength of the line. A trend for the internal dispersion of MMH is also derived. |
|---|