Network regions with more compact positive-polarity magnetic features produce both visible coronal plumes and higher, faster transition-region jets.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.SR 2representative citing papers
New GST and SDO observations of bidirectional plasma jets in a sunspot link them to magnetic reconnection triggered by rising filamentary material interacting with horizontal magnetic loops.
citing papers explorer
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On the relation between transition region network jets and coronal plumes
Network regions with more compact positive-polarity magnetic features produce both visible coronal plumes and higher, faster transition-region jets.
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Bidirectional Plasma Jets Driven by Magnetic Reconnection: Observations by GST and SDO
New GST and SDO observations of bidirectional plasma jets in a sunspot link them to magnetic reconnection triggered by rising filamentary material interacting with horizontal magnetic loops.