Shape and position of Earth’s bow shock near-lunar orbit based on ARTEMIS data

• 作 者: LIU Ji SHI QuanQi TIAN AnMin L
• 机 构: SchoolofSpaceScienceandPhysics,StateKeyLaboratoty,InstituteofSpaceWeather,SchoolofEarthandSpaceScien
• 出 处: 中国科学：地球科学英文版
• 发表日期: 2016年8期
• 关键词: Bow shock Interplanetary magnetic field(IMF) MAGNETOSPHERE Solar wind Bow shockI
• 基金项目: supported by the National Natural Science Foundation of China （Grant Nos. 41322031, 41404131, 41574157, 41031065 ＆ 41304129）,the Specialized Research Fund for State Key Laboratories,the Shandong Natur

Earth’s bow shock is the result of interaction between the supersonic solar wind and Earth’s magnetopause. However, data limitations mean the model of the shape and position of the bow shock are based largely on near-Earth satellite data. The model of the