Parker Solar Probe observations indicate intrinsically enhanced transverse magnetic power inside switchbacks at MHD-ion scales, independent of field angle, coinciding with elevated proton temperatures.
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2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
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2026 2verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
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Wave Activity at MHD-ion Scales Associated with Switchbacks
Parker Solar Probe observations indicate intrinsically enhanced transverse magnetic power inside switchbacks at MHD-ion scales, independent of field angle, coinciding with elevated proton temperatures.
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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.