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.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.SR 3representative citing papers
PSP observations identify flux ropes embedded in HCS reconnection exhausts at ~12 Rs, attributed to secondary reconnection and merging.
Nonlinear hybrid models of PSP-observed anisotropic hot-beam ion VDFs produce combined ion-cyclotron and magnetosonic instabilities whose nonlinear stage yields qualitative agreement with observed hammerhead distributions.
citing papers explorer
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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.
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Magnetic flux ropes within reconnection exhausts close to the centers of heliospheric current sheets near the Sun
PSP observations identify flux ropes embedded in HCS reconnection exhausts at ~12 Rs, attributed to secondary reconnection and merging.
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Modeling hot, anisotropic ion beams in the solar wind motivated by the Parker Solar Probe observations near perihelia
Nonlinear hybrid models of PSP-observed anisotropic hot-beam ion VDFs produce combined ion-cyclotron and magnetosonic instabilities whose nonlinear stage yields qualitative agreement with observed hammerhead distributions.