Poster Open Access

The Martian crustal magnetic field as seen from MG and MAVEN

B. Langlais; E. Thébault


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  "@id": "https://doi.org/10.5281/zenodo.1165832", 
  "@type": "CreativeWork", 
  "creator": [
    {
      "@type": "Person", 
      "affiliation": "LPG, CNRS", 
      "name": "B. Langlais"
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      "affiliation": "LPG, CNRS", 
      "name": "E. Th\u00e9bault"
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  ], 
  "datePublished": "2017-12-11", 
  "description": "<p>The magnetic figure of Mars was essentially constrained by the high quality measurements of Mars Global Surveyor (1996-2006). While the orbital parameters of this mission returned repetitive measurements on the night side (2:00 am) at a nearly constant altitude of 400km, the low altitude measurements were very sparse.</p>\n\n<p>The MAVEN mission (since 2014) is on an elliptical orbit around Mars, which provides a wealth of measurements at different local times and altitudes. With now almost three years of available measurements, it is possible to combine MAVEN and MGS observations and to compute a high resolution model of the martian magnetic field.</p>\n\n<p>This new model supersedes previously published models. It is based on Equivalent Source Dipoles (ESD), a discrete approach which benefits from the varying data distribution. It is converted into a spherical harmonics (SH) model which is stable up to degree 137, and can be used to predict the magnetic field at the surface of Mars with an unprecedented accuracy.</p>", 
  "identifier": "https://doi.org/10.5281/zenodo.1165832", 
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  "keywords": [
    "Mars, MAVENS"
  ], 
  "license": "http://creativecommons.org/licenses/by/4.0/legalcode", 
  "name": "The Martian crustal magnetic field as seen from MG and MAVEN", 
  "url": "https://zenodo.org/record/1165832"
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