作者: Hui Tian , Vasyl Yurchyshyn , Hardi Peter , Sami K. Solanki , Peter R. Young
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摘要: Solid evidence of magnetic reconnection is rarely reported within sunspots, the darkest regions with strongest fields and lowest temperatures in solar atmosphere. Using world's largest telescope, 1.6-meter Goode Solar Telescope, we detect prevalent through frequently occurring fine-scale jets H${\alpha}$ line wings at light bridges, bright lanes that may divide dark sunspot core into multiple parts. Many have an inverted Y-shape, shown by models to be typical a unipolar field environment. Simultaneous spectral imaging data from Interface Region Imaging Spectrograph show drives bidirectional flows up 200~km~s$^{-1}$, weakly ionized plasma heated least order magnitude $\sim$80,000 K. Such highly dynamic efficient heating should properly accounted for future modeling efforts sunspots. Our observations also reveal surge-like activity previously above bridges some chromospheric passbands such as has two components: ever-present short surges likely related upward leakage magnetoacoustic waves photosphere, occasionally long fast are obviously caused intermittent jets.