DEM analysis of the 6 September 2011 coronal wave finds 6-8% density and 10-18% temperature increases at the front, indicating heating mechanisms in addition to compressional adiabatic heating.
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Solar wind composition depends strongly on source distance from the open-closed boundary, with enhanced variability and slow-wind signatures concentrated within ~25 Mm of the boundary.
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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DEM analysis of the 6 September 2011 large-scale coronal wave
DEM analysis of the 6 September 2011 coronal wave finds 6-8% density and 10-18% temperature increases at the front, indicating heating mechanisms in addition to compressional adiabatic heating.
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Solar Wind Dependence on Source Distance from the Open-Closed Boundary
Solar wind composition depends strongly on source distance from the open-closed boundary, with enhanced variability and slow-wind signatures concentrated within ~25 Mm of the boundary.
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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.