| タイトル | Structure of the solar chromosphere. II - The underlying photosphere and temperature-minimum region |
| 著者（英） | Avrett, E. H.; Loeser, R.; Vernazza, J. E. |
| 著者所属（英） | Smithsonian Astrophysical Observatory|Harvard Coll. Observatory |
| 発行日 | 1976-01-01 |
| 言語 | eng |
| 内容記述 | The paper presents a non-LTE empirical model of the quiet solar photosphere and the temperature-minimum region. The continuous spectrum computed from this model is in good overall agreement with available disk-center observations throughout the wavelength range from 0.125 to 500 microns. It is found that (1) absolute-intensity measurements are needed in the range between 1 and 2 microns to establish the structure of the deepest observable layers; (2) absolute-intensity or flux measurements are needed in the range between 20 and 200 microns to determine whether the minimum solar temperature occurring between the photosphere and the chromosphere is as low as indicated by present observations or much higher, as recent theoretical predictions indicate; (3) studies of the far-ultraviolet spectrum based on the assumption of LTE can be substantially in error; and (4) line opacity seems to account for the 'missing opacity' in the ultraviolet. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 76A25247 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/443875 |
