Effects of Stellar XUV Spectra on Atmospheric Escape from a Mars-like Planet Orbiting Inactive Low-Mass Stars
Shotaro Sakai1, Akifumi Nakayama2, Kanako Seki3, Naoki Terada4, Hiroyuki Shinagawa5, Ryoya Sakata3, Francois Leblanc6, David Brain7 and Takashi Tanaka5, (1)Keio University, Faculty of Environment and Information Studies, Tokyo, Japan, (2)Rikkyo University, Department of Physics, College of Science, Tokyo, Japan, (3)The University of Tokyo, Research Center for Advanced Science and Technology, Tokyo, Japan, (4)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (5)Kyushu University, International Research Center for Space and Planetary Environmental Science, Fukuoka, Japan, (6)LATMOS/IPSL, CNRS, Sorbonne Université, UVSQ, Paris, France, (7)University of Colorado at Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States