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DOI码：10.1029/2023JA032355
发表刊物：Journal of Geophysical Research: Space Physics
关键字：Relativistic electrons，EMIC waves
摘要：Resonant interactions of relativistic electrons with electromagnetic ion cyclotron (EMIC) waves were previously considered under the cold plasma approximation or in hot plasmas with bi‐Maxwellian distributions. Here, we examine their resonant interactions in hot plasmas with partial shell distributions and find that such distributions can significantly alter the dispersion relation of EMIC waves and thus the corresponding wave‐induced electron pitch angle scattering rates and loss timescales compared to those under the cold plasma assumption. Regardless of wave band and frequency, partial shell distributed hot protons tend to uplift the electron minimum resonant energy, and reduce (raise) the pitch angle scattering rates of electrons at low (high) energies and large (small) pitch angles. Correspondingly, the loss timescales lengthen for low‐energy electrons but shorten for high‐energy electrons. Such tendencies are generally more significant for lowerfrequency EMIC waves and larger shell temperature, anisotropic degree, and concentration
合写作者：Li L. Y.
第一作者：Yu Jiang
论文类型：期刊论文
一级学科：地球物理学
文献类型：期刊
卷号：129
是否译文：否
发表时间：2024-03-21
收录刊物：SCI
发布期刊链接：https://doi.org/10.1029/2023JA032355