Numerical tracing of stochastic Parker spirals yields an angular field line spread of ~25° at 1 AU that narrows to ~4° when integrated backward to the solar source surface at 0.25 AU.
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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 2years
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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Turbulent Diffusion of Magnetic Field Lines in the Heliosphere
Numerical tracing of stochastic Parker spirals yields an angular field line spread of ~25° at 1 AU that narrows to ~4° when integrated backward to the solar source surface at 0.25 AU.
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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.