OBSERVATIONS and theoretical calculations show that a part of protons are reflected by theshock after the interaction between the solar wind and the quasi-perpendicular collisionlessshock with high Much number.These p...OBSERVATIONS and theoretical calculations show that a part of protons are reflected by theshock after the interaction between the solar wind and the quasi-perpendicular collisionlessshock with high Much number.These protons have large velocities in the direction per-pendicular to the magnetic field and move again towards the downstream of shock due to theeffect of gyration.Upon their second encounter with the shock,most of them are展开更多
文摘OBSERVATIONS and theoretical calculations show that a part of protons are reflected by theshock after the interaction between the solar wind and the quasi-perpendicular collisionlessshock with high Much number.These protons have large velocities in the direction per-pendicular to the magnetic field and move again towards the downstream of shock due to theeffect of gyration.Upon their second encounter with the shock,most of them are
