Solar wind protons experience substantial perpendicular, but not parallel, heating from 0.05 to 1 au, reducing the expected adiabatic growth of temperature anisotropy.
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Solar Wind Proton Heating and its Effect on Temperature Anisotropy Evolution between 0.05 and 1 au
Solar wind protons experience substantial perpendicular, but not parallel, heating from 0.05 to 1 au, reducing the expected adiabatic growth of temperature anisotropy.