| タイトル | The Liege-balloon program |
| 本文（外部サイト） | http://hdl.handle.net/2060/19750004667 |
| 著者（英） | Zander, R. |
| 著者所属（英） | Liege Univ. |
| 発行日 | 1974-11-01 |
| 言語 | eng |
| 内容記述 | The Liege-balloon program is intended to make high-spectral resolution observations of the sun in the near- and intermediate infrared regions not accessible from the ground. A description of the equipment, followed by a summary of the data obtained till now is presented. Except for ozone whose maximum of concentration lies near 25 Km altitude, the residual mass distribution of the other mentioned molecules decreases with altitude. This is a self-explanatory argument for carrying out spectroscopic observations from platforms transcending the densest layers of the earth's atmosphere. The Liege balloon equipment is primarily intended for very high-resolution solar observations from about 27-30 Km altitude, in all spectral regions between 1.5 and 15.0 microns, not accessible from the ground. |
| NASA分類 | ASTRONOMY |
| レポートNO | 75N12739 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/570409 |
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