| タイトル | On the meteor trail spectra |
| 本文（外部サイト） | http://hdl.handle.net/2060/19880005151 |
| 著者（英） | Shafiev, R. I.; Mukhamednazarov, S.; Maltsev, N. V.; Ovezgeldyev, O. G. |
| 著者所属（英） | Academy of Sciences (USSR) |
| 発行日 | 1987-08-01 |
| 言語 | eng |
| 内容記述 | Meteor radiation appears as a result of collisions between meteoroid atoms and air molecules. Depending on duration, this radiation is usually divided into the following types: radiation of the meteor head; radiation of a coma surrounding or immediately following the meteor head; radiation of a trail formed as a result of fragments lagging behind or by the afterglow; and radiation of a meteor train forming from a tail as a result of various chemical and dynamical processes. To investigate physical processes caused by each of the above types, it is necessary to obtain the corresponding experimental data. The physical processes of the radiation and the measurement of the experimental data is discussed. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 88N14533 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/147841 |
