Magnetic Reconnection as the Driver of the Solar Wind

We present EUV solar observations showing evidence for omnipresent jetting activity driven by small-scale magnetic reconnection at the base of corona. argue that physical mechanism heats and drives wind its source is ubiquitous in form (i.e., a.k.a. jetlets). This activity, like heating coronal plasma, are regardless cycle phase. Each event arises from opposite polarity fields producing a short-lived jet hot plasma Alfv\'en waves into The discrete nature these jetlet events leads to intermittent outflows corona, which homogenize as they propagate away Sun wind. discovery establishes importance stellar atmospheres understanding phenomena such acceleration. Based on previous analyses linking switchbacks network, we also new might provide link between corona switchback phenomenon. These need be put bigger picture role diverse atmosphere.