Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
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At solar minimum, the solar wind's density fluctuation level at 90 to 140 solar radii follows a steep sigmoid profile with latitude, with an equator-to-south-pole reduction ratio of 1.62 plus or minus 0.02, while at solar maximum it appears spherically symmetric.
CIRs form closer to young fast-rotating solar-mass stars, migrate outward as rotation slows, and produced 10^3 to 10^7 times more energetic particles than today during the Hadean period.
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Latitudinal dependence of the solar wind during periods of high and low activity through interplanetary scintillation
At solar minimum, the solar wind's density fluctuation level at 90 to 140 solar radii follows a steep sigmoid profile with latitude, with an equator-to-south-pole reduction ratio of 1.62 plus or minus 0.02, while at solar maximum it appears spherically symmetric.
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Corotating Interaction Regions (CIRs): evolution over a solar lifetime
CIRs form closer to young fast-rotating solar-mass stars, migrate outward as rotation slows, and produced 10^3 to 10^7 times more energetic particles than today during the Hadean period.