Turbulence from mixed-polarity magnetic carpet fields supplies enough dissipated energy to heat the solar chromosphere and lower corona, with gradual heating of spicules by entrained turbulence.
: 2000 , Solar Spicules: A Review of Recent Models and Targets for Future Observations - (Invited Review)
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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Network regions with more compact positive-polarity magnetic features produce both visible coronal plumes and higher, faster transition-region jets.
citing papers explorer
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Turbulence and its Potential Impact on Solar Chromospheric and Coronal Heating
Turbulence from mixed-polarity magnetic carpet fields supplies enough dissipated energy to heat the solar chromosphere and lower corona, with gradual heating of spicules by entrained turbulence.
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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.