作者: Marit Øieroset , David L. Mitchell , Tai D. Phan , Robert P. Lin , Mario H. Acuña
DOI: 10.1029/2000GL012289
关键词: Bow shock (aerodynamics) 、 Martian 、 Physics 、 Electron temperature 、 Geophysics 、 Solar wind 、 Magnetic field 、 Electron density 、 Interplanetary spaceflight 、 Interplanetary magnetic field
摘要: We present Mars Global Surveyor (MGS) observations of hot diamagnetic cavities upstream the Martian bow shock. The events are characterized by a region turbulent magnetic field, high electron temperature, and densities at or below ambient solar wind density. temperature is flanked layers field density accompanied rotation in interplanetary (IMF). suggest that generated discontinuities interacting with shock, i.e., counterpart to flow anomalies observed Earth's