期刊
SPACE SCIENCE REVIEWS
卷 215, 期 8, 页码 -出版社
SPRINGER
DOI: 10.1007/s11214-019-0617-7
关键词
Auroral phenomena; Dayside aurora; Cusp; Magnetic reconnection; MI-coupling; Energetic particles; Field-aligned currents and current systems; Energetic particle precipitation
资金
- NSF [AGS-1004736]
- National Key R&D Program of China [2018YFC1407303]
- National Natural Science Foundation of China (NSFC) [41774174]
- Science and Technology Facilities Council (STFC), UK [ST/N000749/1]
- Research Council of Norway/CoE [223252/F50]
- NASA's Explorers Program [NNG12FA45C, NNG12FA42I]
- STFC [ST/N000749/1] Funding Source: UKRI
Dayside aurora is related to processes in the dayside magnetosphere and especially at the dayside magnetopause. A number of dayside aurora phenomena are driven by reconnection between the solar wind interplanetary magnetic field and the Earth's internal magnetic field at the magnetopause. We summarize the properties and origin of aurora at the cusp foot point, High Latitude Dayside Aurora (HiLDA), Poleward Moving Auroral Forms (PMAFs), aurora related to traveling convection vortices (TCV), and throat aurora. Furthermore we discuss dayside diffuse aurora, morning side diffuse aurora spots, and shock aurora.
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