| タイトル | Does wrinkle ridge formation on Mars involve most of the lithosphere |
| 本文（外部サイト） | http://hdl.handle.net/2060/19910013679 |
| 著者（英） | Suppe, J.; Plescia, J. B.; Golombek, M. P.; Narr, W.; Banerdt, B. |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 1990-01-01 |
| 言語 | eng |
| 内容記述 | Recent work on the origin of wrinkle ridges suggests that they are compressional tectonic features whose subsurface structure is not understood. Some characteristics of Martian wrinkle ridges are reviewed which suggest that they are the surface expression of thrust faults that extend through much of the lithosphere. |
| NASA分類 | LUNAR AND PLANETARY EXPLORATION |
| レポートNO | 91N22992 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/132723 |
