| タイトル | The coronal-sounding experiment |
| 著者（英） | Edenhofer, P.; Asmar, S. W.; Volland, H.; Brenkle, J. P.; Paetzold, M.; Bird, M. K. |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 1992-01-01 |
| 言語 | eng |
| 内容記述 | The main science objective of the Ulysses Solar Corona Experiment is to derive the plasma parameters of the solar atmosphere using established coronal-sounding techniques. Applying appropriate model assumptions, the 3D electron density distribution will be determined from dual-frequency ranging and Doppler measurements recorded at the NASA Deep Space Network during the solar conjunctions. Multi-station observations will be used to derive the plasma bulk velocity at solar distances where the solar wind is expected to undergo its greatest acceleration. As a secondary objective profiting from the favorable geometry during Jupiter encounter, radio-sounding measurements will yield a unique cross-scan of the electron density in the Io Plasma Torus. |
| NASA分類 | SPACECRAFT INSTRUMENTATION |
| レポートNO | 92A24319 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/329461 |
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