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机译:The Relationship Between Photoelectron Boundary and Steep Electron Density Gradient on Mars: MAVEN Observations
Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China;
Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing, Peoples R China;
Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R ChinaMax Planck Inst Solar Syst Res, Gottingen, GermanySun Yat Sen Univ, Sch Atmospher Sci, Zhuhai, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Key Lab Lunar & Deep Space Explorat, Beijing, Peoples R ChinaChinese Acad Sci, Inst Earth Sci, Beijing, Peoples R ChinaUniv Colorado, LASP, Boulder, CO 80309 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USANASA, Planetary Magnetospheres Lab, Solar Syst Explorat Div, Goddard Space Flight Ctr, Greenbelt, MD USA;
Mars; photoelectron boundary; steep electron density gradient; SOLAR-WIND INTERACTION; CRUSTAL MAGNETIC-FIELD; MARTIAN IONOSPHERE; RADAR SOUNDINGS; ENERGY PEAKS; 1ST; MHD; IONOPAUSE; ASPERA-3; VENUS;