The first kinetic simulation of expanding Alfvénic turbulence shows formation of parallel suprathermal electron power-law tails that persist through firehose instability.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Statistical analysis shows solar energetic electrons rarely cross the heliospheric current sheet unless the source or spacecraft is close to it.
citing papers explorer
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Formation of Suprathermal Electron Populations in the Expanding, Turbulent Solar Wind
The first kinetic simulation of expanding Alfvénic turbulence shows formation of parallel suprathermal electron power-law tails that persist through firehose instability.
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Do Solar Energetic Electrons cross the Heliospheric Current Sheet? - A Statistical Study
Statistical analysis shows solar energetic electrons rarely cross the heliospheric current sheet unless the source or spacecraft is close to it.