Martian geomorphology /
The latest Mars missions are returning data of unprecedented fidelity in their representation of the martian surface. New data include images with spatial resolution better than 30 cm per pixel, stereo imaging-derived terrain models with one meter postings, high-resolution imaging spectroscopy, and...
Saved in:
| Other Authors: | |
|---|---|
| Format: | Book |
| Language: | English |
| Published: |
London :
Geological Society,
©2011.
|
| Series: | Geological Society special publication ;
no. 356. |
| Subjects: |
MARC
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| 245 | 0 | 0 | |a Martian geomorphology / |c edited by M.R. Balme [and others]. |
| 260 | |a London : |b Geological Society, |c ©2011. | ||
| 300 | |a 307 pages : |b illustrations (some color), maps (some color) ; |c 26 cm. | ||
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| 490 | 1 | |a Geological Society special publication, |x 0305-8719 ; |v no. 356 | |
| 504 | |a Includes bibliographical references and index. | ||
| 505 | 0 | |a A background to Mars exploration and research -- Morphological and geographical evidence for the origin of Phobos' grooves from HRSC Mars Express images -- Periglacial geomorphology and landscape evolution of the Tempe Terra region, Mars -- Evolution of periglacial landforms in the ancient mountain range of the Thaumasia Highlands, Mars -- Landforms indicative of ground-ice thaw in the northern high latitudes of Mars -- Landscape evolution in Martian mid-latitude regions : insights from analogous periglacial landforms in Svalbard -- Water ice sublimation-related landforms on Mars -- Identifying Martian gully evolution -- The indication of Martian gully formation processes by slope-area analysis -- Fill and spill in Lethe Vallis : a recent flood-routing system in Elysium Planitia, Mars -- Geologically recent water flow inferred in channel systems in the NE Sulci Gordii region, Mars -- Layering and degradation of the Rupes Tenuis unit, Mars : a structural analysis south of Chasma Boreale -- A comparative study of interior layered deposits on Mars. | |
| 520 | |a The latest Mars missions are returning data of unprecedented fidelity in their representation of the martian surface. New data include images with spatial resolution better than 30 cm per pixel, stereo imaging-derived terrain models with one meter postings, high-resolution imaging spectroscopy, and RADAR data that reveal subsurface structure. This book reveals how this information is being used to understand the evolution of martian landscapes. | ||
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| 651 | 0 | |a Mars (Planet) |x Geology. | |
| 650 | 0 | |a Geomorphology. | |
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