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Autor:
Knapmeyer, M., Stähler, S., Plesa, A.‐C., Ceylan, S., Charalambous, C., Clinton, J., Dahmen, N., Durán, C., Horleston, A., Kawamura, T., Kim, D., Li, J., Plasman, M., Zenhäusern, G., Weber, R. C., Giardini, D., Panning, M. P., Lognonné, P., Banerdt, W. B., 2 Institute of Geophysics ETH Zürich Zürich Switzerland, 1 DLR Institute for Planetary Research Berlin Germany, 3 Department of Electrical and Electronic Engineering Imperial College London London UK, 4 Swiss Seismological Service (SED) ETH Zurich Zürich Switzerland, 5 School of Earth Sciences University of Bristol Bristol UK, 6 Université de Paris Institut de physique du globe de Paris CNRS F‐75005 Paris France, 7 Department of Earth, Planetary, and Space Sciences University of California, Los Angeles Los Angeles CA USA, 8 NASA MSFC Huntsville AL USA, 9 Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA
Publikováno v:
Geophysical Research Letters, 50 (7)
The seismic activity of a planet can be described by the corner magnitude, events larger than which are extremely unlikely, and the seismic moment rate, the long‐term average of annual seismic moment release. Marsquake S1222a proves large enough to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::51f1000c73c42d62a0948066c89d3f67
https://hdl.handle.net/20.500.11850/610118
https://hdl.handle.net/20.500.11850/610118