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Diffuse and Pulsating Aurora
Space Science Reviews ( IF 9.1 ) Pub Date : 2020-01-08 , DOI: 10.1007/s11214-019-0629-3
Yukitoshi Nishimura , Marc R. Lessard , Yuto Katoh , Yoshizumi Miyoshi , Eric Grono , Noora Partamies , Nithin Sivadas , Keisuke Hosokawa , Mizuki Fukizawa , Marilia Samara , Robert G. Michell , Ryuho Kataoka , Takeshi Sakanoi , Daniel K. Whiter , Shin-ichiro Oyama , Yasunobu Ogawa , Satoshi Kurita

This chapter reviews fundamental properties and recent advances of diffuse and pulsating aurora. Diffuse and pulsating aurora often occurs on closed field lines and involves energetic electron precipitation by wave-particle interaction. After summarizing the definition, large-scale morphology, types of pulsation, and driving processes, we review observation techniques, occurrence, duration, altitude, evolution, small-scale structures, fast modulation, relation to high-energy precipitation, the role of ECH waves, reflected and secondary electrons, ionosphere dynamics, and simulation of wave-particle interaction. Finally we discuss open questions of diffuse and pulsating aurora.

中文翻译:

漫射和脉动极光

本章回顾了弥散和脉动极光的基本特性和最新进展。弥散和脉动极光通常发生在闭合场线上,并涉及通过波粒相互作用产生的高能电子沉淀。在总结定义、大尺度形态、脉动类型和驱动过程后,我们回顾了观测技术、发生、持续时间、高度、演化、小尺度结构、快速调制、与高能降水的关系、ECH的作用波、反射和二次电子、电离层动力学以及波粒相互作用的模拟。最后,我们讨论弥漫性和脉动极光的开放性问题。
更新日期:2020-01-08
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