| タイトル | Extension of convection modeling into the high-latitude ionosphere - Some theoretical difficulties |
| 著者（英） | Rich, F. J.; Wolf, R. A.; Spiro, R. W. |
| 著者所属（英） | Phillips Lab.|Rice Univ. |
| 発行日 | 1991-09-01 |
| 言語 | eng |
| 内容記述 | The Rice Convection Model (RCM) is extended and merged with empirical models so as to cover the entire high-latitude ionosphere with the aim of providing precipitation and electric field inputs for ionosphere and thermosphere modelers and producing a model in which the boundaries of the precipitation and electric field patterns maintain physically consistent relationships to each other. The computed auroral electron energy flux, plotted as a function of latitude, exhibited an exaggerated two-peak structure. When no floor was placed under the precipitation rate, the minimum between the two peaks was much too deep to be consistent with typical observations. The regions of excessively weak precipitation map to equatorial distances of 15-35 RE and thus to the regions of the plasma sheet that were not included in previous self-consistent convection calculations. |
| NASA分類 | GEOPHYSICS |
| レポートNO | 92A13820 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/331159 |
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