The Marsquake Service: Securing Daily Analysis of SEIS Data and Building the Martian Seismicity Catalogue for InSight

被引:49
作者
Clinton, J. [1 ]
Giardini, D. [2 ]
Bose, M. [1 ,2 ]
Ceylan, S. [2 ]
van Driel, M. [2 ]
Euchner, F. [2 ]
Garcia, R. F. [3 ]
Kedar, S. [4 ]
Khan, A. [2 ]
Stahler, S. C. [2 ]
Banerdt, B. [4 ]
Lognonne, P. [5 ]
Beucler, E. [6 ]
Daubar, I. [4 ]
Drilleau, M. [5 ]
Golombek, M. [4 ]
Kawamura, T. [5 ]
Knapmeyer, M. [7 ]
Knapmeyer-Endrun, B. [8 ]
Mimoun, D.
Mocquet, A. [6 ]
Panning, M. [4 ]
Perrin, C. [5 ]
Teanby, N. A. [9 ]
机构
[1] Swiss Fed Inst Technol, Swiss Seismol Serv, Zurich, Switzerland
[2] Swiss Fed Inst Technol, Inst Geophys, Zurich, Switzerland
[3] Toulouse Univ, ISAE SUPAERO, Toulouse, France
[4] CALTECH, Jet Prop Lab, Pasadena, CA USA
[5] Paris VII Denis Diderot Univ, Sorbonne Paris Cite, Inst Phys Globe Paris, CNRS, Paris, France
[6] Univ Nantes, CNRS UMR 6112, Lab Planetol & Geodynam, Nantes, France
[7] DLR Inst Planetary Res, Berlin, Germany
[8] Univ Cologne, Seismol Observ Bensberg, Cologne, Germany
[9] Univ Bristol, Sch Earth Sci, Queens Rd, Bristol BS8 1RJ, Avon, England
基金
美国国家航空航天局; 瑞士国家科学基金会;
关键词
InSight; SEIS; Marsquakes; Martian seismicity; Impacts; Seismicity catalogue; MOMENT-FREQUENCY RELATION; CERBERUS FOSSAE; SINGLE-STATION; INTERIOR STRUCTURE; METEORITE IMPACTS; THERMAL EVOLUTION; SOURCE PARAMETERS; TECTONIC ACTIVITY; ELYSIUM PLANITIA; SOURCE INVERSION;
D O I
10.1007/s11214-018-0567-5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The InSight mission expects to operate a geophysical observatory on Mars for at least two Earth years from late 2018. InSight includes a seismometer package, SEIS. The Marsquake Service (MQS) is created to provide a first manual review of the seismic data returned from Mars. The MQS will detect, locate, quantify and classify seismic events, whether tectonic or impact in origin. Asuite of new and adapted methodologies have been developed to allow location and quantification of seismic events at the global scale using a single station, and a software framework has been developed that supports these methods. This paper describes the expected signals that will be recorded by SEIS, the methods used for their identification and interpretation, and reviews the planned MQS operational procedures. For each seismic event, the MQS will locate events using all available body and surface phases, using the best estimates of the Martian structure, which will become more accurate as more Martian marsquakes are identified and located. The MQS will curate the Mars seismicity catalogue, with all events being relocated to use revised suites of structure models as they are introduced.
引用
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页数:33
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