On the nature of the transition region from the chromosphere to the corona of the Sun

By H. Peter. 2001

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The FIP and Inverse FIP Effects in Solar and Stellar Coronae (2015, background): “aves The Alfv´en wave levels suggested above are similar to those observed in solar ﬂares (e.g. Alexander et al., 1998), but higher than those usually considered and observed in the solar corona (cf. Peter, 2001; De Pontieu et al., 2007; Peter, 2010; McIntosh et al., 2011). The predicted slow mode w”
Coronal Holes and the High-Speed Solar Wind (2002, background): “The topologically complex nature of the transition region, probably made up of loops and open “funnels” with varying spatial scales, is being further elucidated by this instrument (Peter 2000, 2001; Hackenberg et al. 2000).”
On Solving the Coronal Heating Problem (2005, background): “…in the chromosphere (Schrijver, 2005), in low-lying cool (T < 0.2 MK) loops (Antiochos and Noci, 1986; Feldman, Widing, and Warren, 1999, 2000; Peter, 2001), and in the lower legs of warm and hot loops (Aschwanden, Schrijver, and Alexander, 2001), but higher altitude reconnection must play an…”