| タイトル | Offset, tilted dipole models of Uranian smooth high-frequency radio emission |
| 著者（英） | Romig, Joseph H.; Schweitzer, Andrea E.; Evans, David R.; Sawyer, Constance B.; Warwick, James W. |
| 著者所属（英） | Radiophysics, Inc. |
| 発行日 | 1990-09-01 |
| 言語 | eng |
| 内容記述 | The smooth high-frequency (SHF) component of the radio emission detected during the Voyager 2 encounter with Uranus (January 1986) is studied. An offset tilted dipole (OTD) investigation of the SHF emission at L shells is carried out within the range of the bursty source locations. A viable high L shell model is presented. It is suggested that Miranda, which reaches a minimum L shell at L = 5, may be related to the timing of several types of radio emissions. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 90A50422 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/353744 |
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