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 Cosmic Research
Hinode 6