Solar Wind Temperature Isotropy

P. H. Yoon, J. Seough, C. S. Salem, K. G. Klein

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

Reliable models of the solar wind in the near-Earth space environment may constrain conditions close to the Sun. This is relevant to NASA's contemporary innerheliospheric mission Parker Solar Probe. Among the outstanding issues is how to explain the solar wind temperature isotropy. Perpendicular and parallel proton and electron temperatures near 1 AU are theoretically predicted to be unequal, but in situ observations show quasi-isotropy sufficiently below the instability threshold condition. This has not been satisfactorily explained. The present Letter shows that the dynamical coupling of electrons and protons via collisional processes and instabilities may contribute toward the resolution of this problem.

Original languageEnglish (US)
Article number145101
JournalPhysical review letters
Volume123
Issue number14
DOIs
StatePublished - Oct 3 2019

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isotropy
solar wind
solar probes
Earth environment
protons
aerospace environments
electron energy
thresholds
temperature
electrons

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Solar Wind Temperature Isotropy. / Yoon, P. H.; Seough, J.; Salem, C. S.; Klein, K. G.

In: Physical review letters, Vol. 123, No. 14, 145101, 03.10.2019.

Research output: Contribution to journalArticle

Yoon, P. H. ; Seough, J. ; Salem, C. S. ; Klein, K. G. / Solar Wind Temperature Isotropy. In: Physical review letters. 2019 ; Vol. 123, No. 14.
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