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Magnetosheath High‐Speed Jet Drives Multiple Auroral Arcs Near Local Noon

Abstract Magnetosheath High‐Speed Jets (HSJs) are transient disturbances characterized by increased dynamic pressure. They can cause various geoeffects, including ultra‐low‐frequency (ULF) waves and auroras. Theoretically, when ULF waves propagate into the ionosphere as Alfvén waves, they can accele...

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Bibliographic Details
Main Authors: Hui‐Xuan Qiu, De‐Sheng Han, Run Shi, Jianjun Liu
Format: Artigo
Language:Inglês
Published: Wiley 2024-10-01
Series:AGU Advances
Subjects:
Online Access:https://doi.org/10.1029/2024AV001197
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