Dust and sand transport on Mars
Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review
Dust is an active and abundant component both in the Martian atmosphere and on its surface. Its origin, evolution and transport mechanisms are poorly understood yet of great scientific and technical importance to the study and understanding this planet. Current research will be presented in which earth based simulations are performed at a unique wind tunnel facility. This work is complemented by computer modelling and the development of new instrumentation for Martian surface studies. It is specifically hoped to learn more about dust electrification, aggregation, the processes of suspension (entrainment) and deposition.
Original language | English |
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Title of host publication | Powders Grains - Proc. Int. Conf. Micromechanics Granular Media |
Number of pages | 4 |
Publication date | 1 Dec 2005 |
Pages | 963-966 |
ISBN (Print) | 0415383471, 9780415383479 |
Publication status | Published - 1 Dec 2005 |
Event | 5th International Conference on the Micromechanics of Granular Media: Powders and Grains 2005 - Stuttgart, Germany Duration: 18 Jul 2005 → 22 Jul 2005 |
Conference
Conference | 5th International Conference on the Micromechanics of Granular Media: Powders and Grains 2005 |
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Land | Germany |
By | Stuttgart |
Periode | 18/07/2005 → 22/07/2005 |
Series | Powders and Grains 2005 - Proceedings of the 5th International Conference on Micromechanics of Granular Media |
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Volume | 2 |
ID: 230187536