A New Model of the Crustal Magnetic Field of Mars Using MGS and MAVEN

While devoid of an active magnetic dynamo field today, Mars possesses a remanent magnetic field that may reach several thousand nanoteslas locally. The exact origin and the events that have shaped the crustal magnetization remain largely enigmatic. Three magnetic field data sets from two spacecraft...

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Published inJournal of geophysical research. Planets Vol. 124; no. 6; pp. 1542 - 1569
Main Authors Langlais, Benoit, Thébault, Erwan, Houliez, Aymeric, Purucker, Michael E., Lillis, Robert J.
Format Journal Article
LanguageEnglish
Published United States 01.06.2019
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Abstract While devoid of an active magnetic dynamo field today, Mars possesses a remanent magnetic field that may reach several thousand nanoteslas locally. The exact origin and the events that have shaped the crustal magnetization remain largely enigmatic. Three magnetic field data sets from two spacecraft collected over 13 cumulative years have sampled the Martian magnetic field over a range of altitudes from 90 up to 6,000 km: (a) Mars Global Surveyor (MGS) magnetometer (1997–2006), (b) MGS Electron Reflectometer (1999–2006), and (c) Mars Atmosphere and Volatile EvolutioN (MAVEN) magnetometer (2014 to today). In this paper we combine these complementary data sets for the first time to build a new model of the Martian internal magnetic field. This new model improves upon previous ones in several aspects: comprehensive data coverage, refined data selection scheme, modified modeling scheme, discrete‐to‐continuous transformation of the model, and increased model resolution. The new model has a spatial resolution of ∼160 km at the surface, corresponding to spherical harmonic degree 134. It shows small scales and well‐defined features, which can now be associated with geological signatures. Key Points MGS and MAVEN magnetic field measurements are combined into a high‐resolution magnetic field model The new model extends up to SH degree 134, corresponding to 160‐km horizontal resolution at the Martian surface It enables local studies, where geologic and magnetic features can be compared
AbstractList While devoid of an active magnetic dynamo field today, Mars possesses a remanent magnetic field that may reach several thousand nanoteslas locally. The exact origin and the events that have shaped the crustal magnetization remain largely enigmatic. Three magnetic field data sets from two spacecraft collected over 13 cumulative years have sampled the Martian magnetic field over a range of altitudes from 90 up to 6,000 km: (a) Mars Global Surveyor (MGS) magnetometer (1997–2006), (b) MGS Electron Reflectometer (1999–2006), and (c) Mars Atmosphere and Volatile EvolutioN (MAVEN) magnetometer (2014 to today). In this paper we combine these complementary data sets for the first time to build a new model of the Martian internal magnetic field. This new model improves upon previous ones in several aspects: comprehensive data coverage, refined data selection scheme, modified modeling scheme, discrete‐to‐continuous transformation of the model, and increased model resolution. The new model has a spatial resolution of ∼160 km at the surface, corresponding to spherical harmonic degree 134. It shows small scales and well‐defined features, which can now be associated with geological signatures. Key Points MGS and MAVEN magnetic field measurements are combined into a high‐resolution magnetic field model The new model extends up to SH degree 134, corresponding to 160‐km horizontal resolution at the Martian surface It enables local studies, where geologic and magnetic features can be compared
While devoid of an active magnetic field today, Mars possesses a remanent magnetic field which may reach several thousand nT locally. The exact origin, and the events which have shaped the crustal magnetization remain largely enigmatic. Three magnetic field datasets from two spacecraft collected over 13 cumulative years have sampled the martian magnetic field over a range of altitudes from 90 km up to 6000 km: a- Mars Global Surveyor (MGS) magnetometer (1997-2006); b- MGS Electron Reflectometer (1999-2006); c- MAVEN magnetometer (2014-today). In this paper we combine these complementary datasets for the first time to build a new model of the martian internal magnetic field. This new model improves upon previous ones in several aspects: comprehensive data coverage; refined data selection scheme; modified modeling scheme; discrete-to-continuous transformation of the model; increased model resolution. The new model has a spatial resolution of ~ 160 km at the surface, corresponding to spherical harmonic degree 134. It shows small scales and well defined features, which can now be associated with geological signatures.
Author Langlais, Benoit
Thébault, Erwan
Houliez, Aymeric
Lillis, Robert J.
Purucker, Michael E.
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  surname: Thébault
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  givenname: Michael E.
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  surname: Lillis
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  organization: University of California
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Snippet While devoid of an active magnetic dynamo field today, Mars possesses a remanent magnetic field that may reach several thousand nanoteslas locally. The exact...
While devoid of an active magnetic field today, Mars possesses a remanent magnetic field which may reach several thousand nT locally. The exact origin, and the...
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wiley
SourceType Index Database
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StartPage 1542
SubjectTerms crustal field
equivalent source dipoles
magnetic field measurements
Mars crustal magnetization
Mars magnetic field
spherical harmonics
Title A New Model of the Crustal Magnetic Field of Mars Using MGS and MAVEN
URI https://onlinelibrary.wiley.com/doi/abs/10.1029%2F2018JE005854
https://www.ncbi.nlm.nih.gov/pubmed/35096494
Volume 124
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