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Rationale for Seismic Measurements on Mars by a Single StationWe present here some of the scientific objectives which can be achieved by a single seismic station on Mars, equipped with a 3 axis VBB seismometer and a 3 axis Short Period Seismometer. We assume that this station is also equipped with meteorological sensors, including infra-sound and pressure, in order to perform a complete meteorological noise correction. The science objectives are listed in order of increasing difficulty.
Document ID
20030066570
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
P Lognonne
(Institut De Physique Du Globe De Paris Paris, France)
W B Banerdt
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Date Acquired
August 21, 2013
Publication Date
July 25, 2003
Publication Information
Publication: Sixth International Conference on Mars
Publisher: LPI
Subject Category
Geophysics
Report/Patent Number
3225
Meeting Information
Meeting: vSixth International Conference on Mars
Location: Pasadena, CA
Country: US
Start Date: July 20, 2003
End Date: July 25, 2003
Sponsors: Lunar and Planetary Institute
Funding Number(s)
CONTRACT_GRANT: NCC5-679
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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