TY - JOUR
T1 - The Marsquake Service
T2 - Securing Daily Analysis of SEIS Data and Building the Martian Seismicity Catalogue for InSight
AU - Clinton, J.
AU - Giardini, D.
AU - Bose, M.
AU - Ceylan, S.
AU - van Driel, M.
AU - Euchner, F.
AU - Garcia, R. F.
AU - Kedar, S.
AU - Khan, A.
AU - Stahler, S. C.
AU - Banerdt, B.
AU - Lognonne, P.
AU - Beucler, E.
AU - Daubar, I.
AU - Drilleau, M.
AU - Golombek, M.
AU - Kawamura, T.
AU - Knapmeyer, M.
AU - Knapmeyer-Endrun, B.
AU - Mimoun, D.
AU - Mocquet, A.
AU - Panning, M.
AU - Perrin, C.
AU - Teanby, N. A.
PY - 2018/12
Y1 - 2018/12
N2 - 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.
AB - 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.
KW - Impacts
KW - InSight
KW - Marsquakes
KW - Martian seismicity
KW - Seis
KW - Seismicity catalogue
UR - https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=performanshacettepe&SrcAuth=WosAPI&KeyUT=WOS:000452524100001&DestLinkType=FullRecord&DestApp=WOS_CPL
U2 - 10.1007/s11214-018-0567-5
DO - 10.1007/s11214-018-0567-5
M3 - Review article
SN - 0038-6308
VL - 214
JO - Space Science Reviews
JF - Space Science Reviews
IS - 8
M1 - 133
ER -