Plasma and Fusion Research
Volume 21, 1401029 (2026)
Regular Articles
- 1)
- National Institute for Fusion Science, National Institutes of Natural Sciences, Toki, Gifu 509-5292, Japan
- 2)
- The Graduate University for Advanced Studies, SOKENDAI, Toki, Gifu 509-5292, Japan
- 3)
- Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University, Kyoto 606-8502, Japan
Abstract
In a two-ion-species plasma, a magnetosonic wave splits into two distinct modes: a low-frequency mode and a high-frequency mode. Nonlinear solitary waves corresponding to these modes can accelerate heavy ions in a plasma composed of hydrogen (H) and a heavier ion species (denoted by b). In this study, we theoretically examine the dependence of the heavy-ion acceleration on the heavy-ion mass (mb) and the difference between cyclotron frequencies ΩH and Ωb. When the pulse amplitude is fixed, the heavy-ion acceleration weakens as mb increases for both the low- and high-frequency-mode pulses. However, for the low-frequency-mode pulse, a maximum attainable amplitude exists, and this amplitude increases as the ratio ΩH/Ωb becomes larger. Consequently, in a plasma containing heavy ions with larger mb, the low-frequency-mode pulse can have a larger amplitude, leading to the enhancement of the heavy-ion acceleration. These results indicate that the low-frequency-mode pulse can accelerate, for instance, oxygen (O) ions in an H-O plasma more effectively than helium (He) ions in an H-He plasma.
Keywords
magnetosonic wave, solitary wave, two-ion-species plasma, heavy-ion acceleration, Earth’s magnetosphere, comets
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