GSTDTAP  > 气候变化
DOI10.1029/2021GL096796
Magnetotail Ion Structuring by Kinetic Ballooning-Interchange Instability
Evgeny V. Panov; San Lu; Philip L. Pritchett
2022-01-28
发表期刊Geophysical Research Letters
出版年2022
英文摘要

By combining three-probe THEMIS observations and 3-D Particle-in-Cell simulations, we identify key structures on the ion gyroradius scale that occur in connection with ballooning-interchange instability (BICI) heads in the Earth’s magnetotail. The mesoscale structures occur at sites of strong ion velocity shear and vorticity where the thermal ion Larmor radius is about half of the width of the head. Finer structures occur at the smaller scales characterizing the wavelength of the electromagnetic ion cyclotron waves generated at the heads. These two processes act to erode and thin the current sheet, thereby forming a local magnetotail configuration that is favorable for reconnection.

领域气候变化
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被引频次:5[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/346038
专题气候变化
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Evgeny V. Panov,San Lu,Philip L. Pritchett. Magnetotail Ion Structuring by Kinetic Ballooning-Interchange Instability[J]. Geophysical Research Letters,2022.
APA Evgeny V. Panov,San Lu,&Philip L. Pritchett.(2022).Magnetotail Ion Structuring by Kinetic Ballooning-Interchange Instability.Geophysical Research Letters.
MLA Evgeny V. Panov,et al."Magnetotail Ion Structuring by Kinetic Ballooning-Interchange Instability".Geophysical Research Letters (2022).
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