Venus's winds and temperatures during the MESSENGER's flyby: An approximation to a three‐dimensional instantaneous state of the atmosphere
Corresponding Author
Institute of Space and Astronautical Science (ISAS/JAXA), Kanagawa, Japan
Correspondence to: J. Peralta,
Search for more papers by this authorInstitute of Space and Astronautical Science (ISAS/JAXA), Kanagawa, Japan
Search for more papers by this authorEscuela Técnica Superior de Ingeniería (UPV/EHU), Bilbao, Spain
Search for more papers by this authorSpace Science Institute, Boulder, Colorado, USA
Search for more papers by this authorSpace Science Institute, Boulder, Colorado, USA
Search for more papers by this authorEscuela Técnica Superior de Ingeniería (UPV/EHU), Bilbao, Spain
Search for more papers by this authorLESIA, Observatoire de Paris/CNRS/UPMC/Université Paris Diderot, Meudon, France
Search for more papers by this authorMax‐Planck‐Institut für Sonnensystemforschung (MPS/MPEG), Göttingen, Germany
European Space Astronomy Centre, Madrid, Spain
Search for more papers by this authorInstitute of Astrophysics and Space Sciences, Observatório Astronómico de Lisboa, Lisbon, Portugal
Search for more papers by this authorUniversity of Tokyo, Tokyo, Japan
Search for more papers by this authorPlanetary Aeronomy, Belgian Institute for Space Aeronomy, Brussels, Belgium
Search for more papers by this authorDepartment of Earth and Planetary Science, Graduate School of Frontier Sciences, University of Tokyo, Tokyo, Japan
Search for more papers by this authorFaculty of Environmental Earth Science, Hokkaido University, Sapporo, Japan
Search for more papers by this authorInstitute of Space and Astronautical Science (ISAS/JAXA), Kanagawa, Japan
Search for more papers by this authorSchool of Engineering, University of Shiga Prefecture, Hikone, Japan
Search for more papers by this authorInstitute of Astrophysics and Space Sciences, Observatório Astronómico de Lisboa, Lisbon, Portugal
Search for more papers by this authorBritish Astronomical Association, London, UK
Search for more papers by this authorCorresponding Author
Institute of Space and Astronautical Science (ISAS/JAXA), Kanagawa, Japan
Correspondence to: J. Peralta,
Search for more papers by this authorInstitute of Space and Astronautical Science (ISAS/JAXA), Kanagawa, Japan
Search for more papers by this authorEscuela Técnica Superior de Ingeniería (UPV/EHU), Bilbao, Spain
Search for more papers by this authorSpace Science Institute, Boulder, Colorado, USA
Search for more papers by this authorSpace Science Institute, Boulder, Colorado, USA
Search for more papers by this authorEscuela Técnica Superior de Ingeniería (UPV/EHU), Bilbao, Spain
Search for more papers by this authorLESIA, Observatoire de Paris/CNRS/UPMC/Université Paris Diderot, Meudon, France
Search for more papers by this authorMax‐Planck‐Institut für Sonnensystemforschung (MPS/MPEG), Göttingen, Germany
European Space Astronomy Centre, Madrid, Spain
Search for more papers by this authorInstitute of Astrophysics and Space Sciences, Observatório Astronómico de Lisboa, Lisbon, Portugal
Search for more papers by this authorUniversity of Tokyo, Tokyo, Japan
Search for more papers by this authorPlanetary Aeronomy, Belgian Institute for Space Aeronomy, Brussels, Belgium
Search for more papers by this authorDepartment of Earth and Planetary Science, Graduate School of Frontier Sciences, University of Tokyo, Tokyo, Japan
Search for more papers by this authorFaculty of Environmental Earth Science, Hokkaido University, Sapporo, Japan
Search for more papers by this authorInstitute of Space and Astronautical Science (ISAS/JAXA), Kanagawa, Japan
Search for more papers by this authorSchool of Engineering, University of Shiga Prefecture, Hikone, Japan
Search for more papers by this authorInstitute of Astrophysics and Space Sciences, Observatório Astronómico de Lisboa, Lisbon, Portugal
Search for more papers by this authorBritish Astronomical Association, London, UK
Search for more papers by this author


