The influence of local topography for wind direction on Mars: two examples of dune fields in crater basins

Author:

Cardinale Marco1,Komatsu Goro1,Silvestro Simone2,Tirsch Daniela3

Affiliation:

1. International Research School of Planetary Sciences; Università G. D'Annunzio; Pescara; Italy

2. SETI Institute - Carl Sagan Center; Mountain View; CA; USA

3. German Aerospace Center (DLR); Institute of Planetary Research; Berlin; Germany

Publisher

Wiley

Subject

Earth and Planetary Sciences (miscellaneous),Earth-Surface Processes,Geography, Planning and Development

Reference38 articles.

1. Morphology and distribution of common “sand” dunes on Mars: comparison with the Earth;Breed;Journal of Geophysical Research,1979

2. Cardinale M Komatsu G Pasculli A 2010 Mare Tyrrenium Region: analysis of dark sand dunes and wind direction interpretations Proceedings, Lunar Planetary Science Conference

3. Orbital observations of contemporary dune activity in Endeavour Crater, Meridiani Planum, Mars;Chojnacki;Journal of Geophysical Research,2011

4. Results from the Mars Global Surveyor Thermal Emission Imaging Spectrometer;Christensen;Science,1998

5. Mars Global Surveyor Thermal Emission Spectrometer experiment: investigation description and surface science results;Christensen;Journal of Geophysical Research,2001

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