Diffuse and Pulsating Aurora

被引：0
作者：
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
机构：
[1] Boston University,Department of Electrical and Computer Engineering and Center for Space Physics
[2] University of New Hampshire,Space Science Center
[3] Tohoku University,Department of Geophysics, Graduate School of Science
[4] Nagoya University,Institute for Space Earth Environmental Research
[5] University of Calgary,Department of Physics and Astronomy
[6] The University Centre in Svalbard,Department of Arctic Geophysics
[7] Birkeland Centre for Space Science,Department of Communication Engineering and Informatics
[8] University of Electro-Communications,Department of Astronomy
[9] NASA Goddard Space Flight Center,Department of Physics and Astronomy
[10] University of Maryland,Space Physics and Astronomy Research Unit
[11] National Institute of Polar Research (NIPR),undefined
[12] SOKENDAI,undefined
[13] University of Southampton,undefined
[14] National Institute of Polar Research,undefined
[15] University of Oulu,undefined
来源：
Space Science Reviews | 2020年 / 216卷
关键词：
Pulsating aurora; Diffuse aurora; Wave-particle interaction; Whistler-mode chorus; Energetic electron precipitation;
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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.
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  • [71] Lanchester B.S.(2016)Amplitude dependence of frequency sweep rates of whistler mode chorus emissions Earth Planets Space 68 857-387
  • [72] Marklund G.(2018)Effect of the background magnetic field inhomogeneity on generation processes of whistler-mode chorus and hiss-like broadband emissions J. Geophys. Res. Space Phys. 123 2210-9201
  • [73] Whiter D.(2019)Electron hybrid code simulation of whistler-mode chorus generation with real parameters in the Earth’s inner magnetosphere J. Geophys. Res. Space Phys. 124 6877-1347
  • [74] Dahlgren H.(2018)Dependence of generation of whistler-mode chorus emissions on the temperature anisotropy and density of energetic electrons in the Earth’s inner magnetosphere Geophys. Res. Lett. 45 575-2766
  • [75] Ivchenko N.(1966)Tracking the region of high correlation between pulsating aurora and chorus: simultaneous observations with Arase satellite and ground-based all-sky imager in Russia J. Geophys. Res. 71 205-7736
  • [76] Lanchester B.S.(2017)Density depletions associated with enhancements of electron cyclotron harmonic emissions: an ERG observation Geophys. Res. Lett. 44 1029-1554
  • [77] Dahlgren H.(1988)Limits on stably trapped particle fluxes Planet. Space Sci. 36 1106-11247
  • [78] Lanchester B.S.(2015)Is diffuse aurora driven from above or below? Space Sci. Rev. 189 59-10748
  • [79] Ivchenko N.(2017)Ionospheric conductivities, electric fields and currents associated with auroral substorms measured by the EISCAT radar J. Geophys. Res. Space Phys. 122 7214-259
  • [80] Whiter D.K.(2001)The CASSIOPE/e-POP Suprathermal Electron Imager (SEI) J. Geophys. Res. 106 1602-3353
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