High-speed streams from coronal holes and the accelerating mechanism of the solar wind

DOI10.1080/03091928208208962zbMath0493.76120OpenAlexW2058470502WikidataQ114640702 ScholiaQ114640702MaRDI QIDQ3956680

Wen-rui Hu

Publication date: 1982

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: http://dspace.imech.ac.cn/handle/311007/39966

zbMATH Keywords

solar windcoronal holeschromospheregeneral Mach equationhigh-speed streams

Mathematics Subject Classification ID

Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (2)

The influence of momentum addition on the acceleration of the solar and stellar winds ⋮ High speed flows and shock waves in astrophysical problems

Cites Work

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