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Inversion of gravity and magnetic field data for Tyrrhena Patera

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dc.contributor.author Milbury, C.
dc.contributor.author Schubert, G.
dc.contributor.author Raymond, C. A.
dc.contributor.author Smrekar, S. E.
dc.date.accessioned 2013-08-07T19:41:04Z
dc.date.available 2013-08-07T19:41:04Z
dc.date.issued 2011-03-07
dc.identifier.citation 42 Lunar and Planetary Institute Conference, Woodlands, Texas, March 7–11, 2011 en_US
dc.identifier.clearanceno 11-0895
dc.identifier.uri http://hdl.handle.net/2014/43453
dc.description.abstract Tyrrhena Patera is located to the southeast/northeast of the Isidis/Hellas impact basin. It was geologically active into the Late Amazonian, although the main edifice was formed in the Noachian (~3.7-4.0 Ga) [1]. Tyrrhena Patera and the surrounding area contain gravity and magnetic anomalies that appear to be correlated (see Fig. 1). The results presented here are for the anomalies 1a and 1b (closest to Tyrrhena Patera), however other anomalies in this region have been modeled and will be presented at the conference. The Mars Global Surveyor (MGS) free-air gravity signature of Tyrrhena Patera has been studied by [2], who inferred the existence of an extinct magma chamber below it. The magnetic signature has been mapped by [3], who compared electron reflectometer data, analogous to the total magnetic field, for Syrtis Major and Tyrrhena Patera and argued for demagnetization of both volcanoes. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011. en_US
dc.subject Mars en_US
dc.subject dynamo en_US
dc.subject volcanism en_US
dc.subject magnetic anomaly en_US
dc.title Inversion of gravity and magnetic field data for Tyrrhena Patera en_US
dc.type Preprint en_US


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