DKIST VBI observations identify 30 spicule events triggered by microfilaments as small as 0.17 Mm, revealing two morphological classes and occasional twisting motions.
Title resolution pending
4 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 4representative citing papers
Frequent EUV microflashes at solar plume bases, each releasing ~10^24 erg, are identified as a new unipolar network event and suggested as a candidate mechanism to power the open corona and solar wind.
Network regions with more compact positive-polarity magnetic features produce both visible coronal plumes and higher, faster transition-region jets.
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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Observational Evidence of Solar Spicules Associated with Microfilament Eruptions Using DKIST
DKIST VBI observations identify 30 spicule events triggered by microfilaments as small as 0.17 Mm, revealing two morphological classes and occasional twisting motions.
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Extreme Ultraviolet Microflashes at Plume Bases: A Candidate for Powering the Corona and Solar Wind?
Frequent EUV microflashes at solar plume bases, each releasing ~10^24 erg, are identified as a new unipolar network event and suggested as a candidate mechanism to power the open corona and solar wind.
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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.