Monitoring Aurora in Day Light Side of the Earth in Relation to Solar Plasma Flow
This is a note to aurora in day light side of the earth in relation to the solar plasma flow.The solar plasma flow in a super high speed forces to form a shock front just in front of the magnetopause between the sun and the earth.The intrusion of the electron into the aurora oval zone along the magnetic line releases its energy to form a visible aurora.It is up-dated what process is reasonable to see the coloring of the interested aurora.An additional notice is given to see a non-natural energy release for a dark red sky in the subtropical zone on the ocean.Spacecraft monitoring of the planets in the solar system is also introduced in short.
Shigehisa Nakamura
Kyoto University,Japan
国际会议
Progress in Electromagnetics Research Symposium 2011(2011年电磁学研究新进展学术研讨会)
苏州
英文
717-720
2011-09-01(万方平台首次上网日期,不代表论文的发表时间)