Simulations of the magnetic properties experiment on Mars Exploration Rovers

被引：2
|
作者：
Gunnlaugsson, H. P.
Worm, E. S.
Bertelsen, P.
Goetz, W.
Kinch, K.
Madsen, M. B.
Merrison, J. P.
Nornberg, P.
机构：
[1] Aarhus Univ, Inst Phys & Astron, DK-8000 Aarhus C, Denmark
[2] Univ Copenhagen, Ctr Planetary Sci, DK-2100 Copenhagen O, Denmark
[3] Max Planck Solar Syst Res, D-37191 Katlenburg Lindau, Germany
[4] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
[5] Aarhus Univ, Dept Earth Sci, DK-8000 Aarhus C, Denmark
来源：
HYPERFINE INTERACTIONS | 2005年 / 166卷 / 1-4期
关键词：
dust on Mars; magnetite; olivine basalt;
D O I：
10.1007/s10751-006-9334-1
中图分类号：
O64 [物理化学（理论化学）、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号：
070203 ; 070304 ; 081704 ; 1406 ;
摘要：
We present some of the main findings from simulation studies of the Magnetic Properties Experiment on the Mars Exploration Rovers. The results suggest that the dust has formed via mechanical breakdown of surface rocks through the geological history of the planet, and that liquid water need not have played any significant role in the dust formation processes.
引用
收藏
页码：555 / 560
页数：6
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