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 2representative citing papers
A new source alignment technique applied to PSP and SO data reveals the solar wind speed increases by an average of 45% per radial decade between the spacecraft, indicating ongoing acceleration beyond 15 solar radii.
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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On the Radial Evolution of the Solar Wind : The Source Alignment Method Applied to Parker Solar Probe and Solar Orbiter Observations
A new source alignment technique applied to PSP and SO data reveals the solar wind speed increases by an average of 45% per radial decade between the spacecraft, indicating ongoing acceleration beyond 15 solar radii.