Double Beam Instability for the Mercury Upstream Waves

Mercury shock-upstream region is plasma physically of great interest, as the solar wind plasma may encounter two ion beams, forming a double-beam plasma system. Properties of the double-beam instability are studied semianalytically using the magnetoionic theory (cold plasma waves including beams), s...

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Bibliographic Details
Main Authors: Y. Narita, U. Motschmann, H. Comişel, D. Schmid
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adc1bc
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