Abstract
Ever since the “direct evidence” of magnetic reconnection in solar wind has been proposed by Gosling et al. (2005a), many reconnection exhausts are reported (Gosling et al. 2005a, b; Davis et al. 2006; Phan et al. 2006; Gosling et al. 2007a, b; Huttunen et al. 2007; Lavraud et al. 2009; Tian et al. 2010; Wang et al. 2010; Gosling 2011; Xu et al. 2011).
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