| タイトル | The solar ionisation rate deduced from Ulysses measurements and its implications to interplanetary Lyman alpha-intensity |
| 著者（英） | Summanen, T.; Kyroelae, E. |
| 著者所属（英） | Finnish Meteorological Inst. |
| 発行日 | 1995-06-30 |
| 言語 | eng |
| 内容記述 | We have developed a computer code which can be used to study 3-dimensional and time-dependent effects of the solar cycle on the interplanetary (IP) hydrogen distribution. The code is based on the inverted Monte Carlo simulation. In this work we have modelled the temporal behaviour of the solar ionisation rate. We have assumed that during the most of the time of the solar cycle there is an anisotopic latitudinal structure but right at the solar maximum the anisotropy disappears. The effects of this behaviour will be discussed both in regard to the IP hydrogen distribution and IP Lyman a a-intensity. |
| NASA分類 | Astrophysics |
| レポートNO | 96N24899 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/304852 |
