| タイトル | Distribution and size of elements of Saturn's rings as inferred from 12-cm radar observations |
| 本文（外部サイト） | http://hdl.handle.net/2060/19750009171 |
| 著者（英） | Morris, G. A., Jr. |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 1974-01-01 |
| 言語 | eng |
| 内容記述 | A 64m radar antenna was used to observe Saturn's rings at 12.6 cm wavelength, with reduced Doppler spread. The results show a positive radar return corresponding to about a 60 percent return from an isotropic scatterer with the projected area of the rings, allowing for the Cassini division. A radar spectrogram of the rings is shown with power density plotted against Doppler frequency shift. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 75N17243 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/570360 |
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