Diffuse and Pulsating Aurora

被引:77
作者
Nishimura, Yukitoshi [1 ,2 ]
Lessard, Marc R. [3 ]
Katoh, Yuto [4 ]
Miyoshi, Yoshizumi [5 ]
Grono, Eric [6 ]
Partamies, Noora [7 ,8 ]
Sivadas, Nithin [1 ,2 ]
Hosokawa, Keisuke [9 ]
Fukizawa, Mizuki [4 ]
Samara, Marilia [10 ]
Michell, Robert G. [10 ,11 ]
Kataoka, Ryuho [12 ,13 ]
Sakanoi, Takeshi [4 ]
Whiter, Daniel K. [14 ]
Oyama, Shin-ichiro [5 ,15 ,16 ]
Ogawa, Yasunobu [12 ,13 ]
Kurita, Satoshi [5 ]
机构
[1] Boston Univ, Dept Elect & Comp Engn, Boston, MA 02215 USA
[2] Boston Univ, Ctr Space Phys, Boston, MA 02215 USA
[3] Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA
[4] Tohoku Univ, Grad Sch Sci, Dept Geophys, Sendai, Miyagi, Japan
[5] Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi, Japan
[6] Univ Calgary, Dept Phys & Astron, Calgary, AB, Canada
[7] Univ Ctr Svalbard, Dept Arctic Geophys, Longyearbyen, Norway
[8] Birkeland Ctr Space Sci, Bergen, Norway
[9] Univ Electrocommun, Dept Commun Engn & Informat, Tokyo, Japan
[10] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
[11] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[12] NIPR, Tachikawa, Tokyo, Japan
[13] SOKENDAI, Tachikawa, Tokyo, Japan
[14] Univ Southampton, Dept Phys & Astron, Southampton, Hants, England
[15] Natl Inst Polar Res, Tokyo, Japan
[16] Univ Oulu, Space Phys & Astron Res Unit, Oulu, Finland
基金
英国自然环境研究理事会;
关键词
Pulsating aurora; Diffuse aurora; Wave-particle interaction; Whistler-mode chorus; Energetic electron precipitation; WHISTLER-MODE CHORUS; MERIDIAN SCANNING PHOTOMETER; CYCLOTRON HARMONIC-WAVES; OPTICAL OBSERVATIONS; MAGNETIC-FIELD; TEMPORAL CHARACTERISTICS; ELECTRON-PRECIPITATION; THEMIS SPACECRAFT; HIGH-RESOLUTION; ENERGY;
D O I
10.1007/s11214-019-0629-3
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页数:38
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