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Present-­‐day Mars' Seismicity Predicted from 3-­‐ D Thermal Evolution Models of Interior Dynamics

Plesa, A.-C. and Knapmeyer, M. and Golombek, M. (2016) Present-­‐day Mars' Seismicity Predicted from 3-­‐ D Thermal Evolution Models of Interior Dynamics. AGU Fall meeting, 12.-­16. Dec. 2016, San Francisco CA, USA.

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Item URL in elib:https://elib.dlr.de/108495/
Document Type:Conference or Workshop Item (Poster)
Title:Present-­‐day Mars' Seismicity Predicted from 3-­‐ D Thermal Evolution Models of Interior Dynamics
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Plesa, A.-C.ana.plesa (at) dlr.deUNSPECIFIED
Knapmeyer, M.martin.knapmeyer (at) dlr.deUNSPECIFIED
Golombek, M.jet propulsion laboratory, pasadena, ca, usaUNSPECIFIED
Date:2016
Refereed publication:No
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Status:Published
Keywords:Mars' seismicity, thermal evolution, interior dynamics
Event Title:AGU Fall meeting
Event Location:San Francisco CA, USA
Event Type:international Conference
Event Dates:12.-­16. Dec. 2016
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Science and Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Erforschung des Weltraums
DLR - Research theme (Project):R - Vorhaben Exploration des Sonnensystems
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research
Institute of Planetary Research > Planetary Physics
Deposited By: Plesa, Dr. Ana-Catalina
Deposited On:29 Nov 2016 11:16
Last Modified:29 Nov 2016 11:16

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