| タイトル | Scientific Rationale and Requirements for a Global Seismic Network on Mars |
| 本文（外部サイト） | http://hdl.handle.net/2060/19920005731 |
| 著者（英） | Solomon, Sean C.; Anderson, Don L.; Phillips, Roger J.; Okal, Emile A.; Davis, Paul M.; Banerdt, W. Bruce; Butler, Rhett G.; Nakamura, Yosio; Duennebier, Frederick K. |
| 著者所属（英） | Lunar and Planetary Inst. |
| 発行日 | 1991-01-01 |
| 言語 | eng |
| 内容記述 | Following a brief overview of the mission concepts for a Mars Global Network Mission as of the time of the workshop, we present the principal scientific objectives to be achieved by a Mars seismic network. We review the lessons for extraterrestrial seismology gained from experience to date on the Moon and on Mars. An important unknown on Mars is the expected rate of seismicity, but theoretical expectations and extrapolation from lunar experience both support the view that seismicity rates, wave propagation characteristics, and signal-to-noise ratios are favorable to the collection of a scientifically rich dataset during the multiyear operation of a global seismic experiment. We discuss how particular types of seismic waves will provide the most useful information to address each of the scientific objectives, and this discussion provides the basis for a strategy for station siting. Finally, we define the necessary technical requirements for the seismic stations. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 92N14949
NAS 1.26:188806
NASA-CR-188806
LPI-TR-91-02 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/129220 |
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