Network regions with more compact positive-polarity magnetic features produce both visible coronal plumes and higher, faster transition-region jets.
: 1998 , Network Activity and the Evaporative Formation of Polar Plumes
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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Long-term 17 GHz microwave polar brightening shows strong correlations with polar coronal hole area and polar magnetic field strength.
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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Microwave Polar Brightening and Its Connection to Polar Coronal Holes
Long-term 17 GHz microwave polar brightening shows strong correlations with polar coronal hole area and polar magnetic field strength.