作者: K. Staines , A. Balogh , S.W.H. Cowley , P.M. de F. Forster , R.J. Hynds
DOI: 10.1016/0273-1177(91)90016-D
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摘要: Abstract Magnetosonic waves are generated by the instability of new-born cometary water group ion distribution. We investigate energy transfer between components velocity distributions measured at comet Giacobini-Zinner (GZ), caused wave-particle scattering, and compare thermal density ions with waves.