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Study fast plasma flows from the edges of solar active regions discovered with Hinode/EIS (Harra et al., 2008), which are driven by pressure gradient between reconnecting magnetic loops (Baker et al., 2009; Del Zanna et al., 2011) and produce intermediate-speed solar wind streams (van Driel-Gesztelyi et al., 2012). Study active region expansion (Uchida et al., 1992).

 

To be moved and be integrated under 1.1.2 Source regions of the slow solar wind. Already planned in L_SMALL_HRES_HCAD_Slow-Wind-Connection.