惑星間コロナ質量放出に対する火星の反応に関するMAVEN観測

¹University of Colorado, Boulder, CO, USA. bruce.jakosky@lasp.colorado.edu.
²NASA/Goddard Space Flight Center, Greenbelt, MD, USA.
³University of California at Berkeley, Berkeley, CA, USA.
⁴University of Colorado, Boulder, CO, USA.
⁵University of Iowa, Iowa City, IA, USA.
⁶Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
⁷University of Michigan, Ann Arbor, MI, USA.
⁸University of California at Los Angeles, Los Angeles, CA, USA.
⁹CNRS-Institut de Recherche en Astrophysique et Planétologie (IRAP), Toulouse, France. University Paul Sabatier, Toulouse, France.
¹⁰Swedish Institute of Space Physics, Uppsala, Sweden.
¹¹NASA/Johnson Space Center, Houston, TX, USA.
¹²National Institute of Aerospace, Hampton, VA, USA.
¹³Laboratoire atmosphères, milieux et observations spatiales (LATMOS)-CNRS, Paris, France.
¹⁴Boston University, Boston, MA, USA.
¹⁵University of Kansas, Lawrence, KS, USA.
¹⁶Computational Physics, Inc., Boulder, CO, USA.
¹⁷Wright State University, Dayton, OH, USA.
¹⁸University of Arizona, Tucson, AZ, USA.
¹⁹Nagoya University, Nagoya, Japan.
²⁰Naval Research Laboratory, Washington, DC, USA.
²¹North Carolina State University, Raleigh, NC, USA.

まとめ

火星は,大気結合とイオン損失により,大気を宇宙に失いました. 火星大気と揮発性進化 (MAVEN) ミッションは,太陽のイベント中にイオン脱出を研究し,火星の薄い大気を説明する損失率を高めました.

まとめ