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• W1998577440 abstract "The present study reveals for the first time the existence of bidirectional jets, which are a signature of magnetic reconnection, occurring along coronal hole boundaries. The Solar Ultraviolet Measurement of Emitted Radiation spectrometer observations obtained in the N IV 765.15 Å (1.3 × 105 K) and Ne VIII 770.42 Å (6 × 105 K) emission lines in an equatorial extension of a polar coronal hole, known as the Elephant's Trunk coronal hole, show small regions of a few arcseconds size with strong blue- and redshifted emission reaching Doppler shifts of up to 150 km s-1, i.e., bidirectional jets. The jets' number density along coronal hole boundaries was found to be about 4-5 times higher with respect to the quiet Sun." @default.
• W1998577440 created "2016-06-24" @default.
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• W1998577440 date "2004-02-12" @default.
• W1998577440 modified "2023-09-30" @default.
• W1998577440 title "Evidence of Magnetic Reconnection along Coronal Hole Boundaries" @default.
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• W1998577440 doi "https://doi.org/10.1086/383030" @default.
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