Turbulence-driven Solar Wind Heating and Energization of Pickup Protons in the Outer Heliosphere

We improve and extend the "dominant turbulence" model of Isenberg et al., which describes the turbulent heating of the distant solar wind by the dissipation of wave energy generated by the isotropization of interstellar pickup protons. We first modify some of the detailed expressions in Is...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 623; no. 1; pp. 502 - 510
Main Author Isenberg, Philip A
Format Journal Article
LanguageEnglish
Published Chicago, IL IOP Publishing 10.04.2005
University of Chicago Press
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