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Solar Coronal Jets: Observations, Theory, and Modeling
DOI: 10.1007/s11214-016-0260-5 Bibcode: 2016SSRv..201....1R

Young, P. R.; Curdt, W.; Raouafi, N. E. +13 more

Coronal jets represent important manifestations of ubiquitous solar transients, which may be the source of significant mass and energy input to the upper solar atmosphere and the solar wind. While the energy involved in a jet-like event is smaller than that of "nominal" solar flares and coronal mass ejections (CMEs), jets share many common propert…

2016 Space Science Reviews
Hinode SOHO 293
Slow Solar Wind: Observations and Modeling
DOI: 10.1007/s11214-016-0264-1 Bibcode: 2016SSRv..201...55A

Li, B.; Harra, L.; Riley, P. +9 more

While it is certain that the fast solar wind originates from coronal holes, where and how the slow solar wind (SSW) is formed remains an outstanding question in solar physics even in the post-SOHO era. The quest for the SSW origin forms a major objective for the planned future missions such as the Solar Orbiter and Solar Probe Plus. Nonetheless, r…

2016 Space Science Reviews
Hinode SOHO 196