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- W1640105 abstract "The visual display of light called the aurora borealis occurs when energetic (1 to 100-keV) electrons, protons, and hydrogen atoms from the Earth`s magnetosphere enter the Earth`s upper atmosphere and collide with the ambient neutral particles. Two kinds of auroras occur in nature: those excited by incident electrons and those excited by incident protons and hydrogen atoms. In this paper, we consider only the latter. The proton-hydrogen aurora may be divided into two altitude regions: high altitudes ({approximately}250 to {approximately}600 km) where charge-changing collisions dominate and energy-loss collisions may be neglected and low altitudes ({approximately}100 to {approximately}250 km) where energy-loss collisions also become important and cause rapid energy degradation. The focus of this review is on the high-altitude region where the one-group approximation is valid." @default.
- W1640105 created "2016-06-24" @default.
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- W1640105 date "1994-12-31" @default.
- W1640105 modified "2023-09-26" @default.
- W1640105 title "Applications to particle transport in the Earth`s aurora" @default.
- W1640105 hasPublicationYear "1994" @default.
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