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Small-Scale Dynamic Aurora

Ryuho Kataoka, C. C. Chaston, D. J. Knudsen, K. A. Lynch, R. L. Lysak, Yan Song, R. Rankin, Kiyoka Murase, Takeshi Sakanoi, J. L. Semeter, Tomo-Hiko Watanabe, Daniel Whiter

2021Space Science Reviews25 citationsDOIOpen Access PDF

Abstract

Small-scale dynamic auroras have spatial scales of a few km or less, and temporal scales of a few seconds or less, which visualize the complex interplay among charged particles, Alfvén waves, and plasma instabilities working in the magnetosphere-ionosphere coupled regions. We summarize the observed properties of flickering auroras, vortex motions, and filamentary structures. We also summarize the development of fundamental theories, such as dispersive Alfvén waves (DAWs), plasma instabilities in the auroral acceleration region, ionospheric feedback instabilities (IFI), and the ionospheric Alfvén resonator (IAR). SUPPLEMENTARY INFORMATION: The online version contains supplementary material available at 10.1007/s11214-021-00796-w.

Topics & Concepts

IonospherePhysicsMagnetospherePlasmaGeophysicsAccelerationAlfvén waveComputational physicsWhistlerScale (ratio)InstabilityAstrophysicsMagnetohydrodynamicsClassical mechanicsMechanicsNuclear physicsQuantum mechanicsIonosphere and magnetosphere dynamicsSolar and Space Plasma DynamicsDust and Plasma Wave Phenomena
Small-Scale Dynamic Aurora | Litcius