Search Publications
Identification of coronal sources of the solar wind from solar images in the EUV spectral range
DOI: 10.1134/S0010952515010074
Bibcode: 2015CosRe..53...47S
Slemzin, V. A.; Shugai, Yu. S.
Methods of localizing coronal sources of the solar wind (SW), such as coronal holes, quasi-stationary fluxes from active regions, and transient sources associated with small-scale active phenomena are considered based on vacuum-ultraviolet (EUV) images of the corona at low solar activity during the initial period of the 24th solar cycle (2010). It…
2015
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Cosmic Research
Hinode
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