作者: E.M. Dubinin , K. Sauer , K. Baumgärtel , R. Lundin
DOI: 10.1016/S0273-1177(97)00525-5
关键词: Physics 、 Martian 、 Solar wind 、 Magnetosphere 、 Magnetosphere of Jupiter 、 Astrophysics 、 Magnetosheath 、 Atmosphere of Mars 、 Astrobiology 、 Population 、 Magnetopause
摘要: Abstract Plasma and magnetic field data from the PHOBOS-2 spacecraft are examined to provide a description of Martian magnetosheath. The addition planetary-ion population hydrogen magnetoplasma strongly modifies characteristics this region. transition shocked solar wind magnetosphere is characterized by appearance new boundaries. magnetosheath filled intense bi-ion magnetoacoustic waves which may evolve multiple shock-like structures.