Radial evolution of the electron distribution functions in the fast solar wind between 0.3 and 1.5 AU-Reference-Cited by-同舟云学术

Radial evolution of the electron distribution functions in the fast solar wind between 0.3 and 1.5 AU

Published:2005-09 Issue:A9 Volume:110 Page:
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Maksimovic M.¹,Zouganelis I.¹,Chaufray J.-Y.¹,Issautier K.¹,Scime E. E.²,Littleton J. E.²,Marsch E.³,McComas D. J.⁴,Salem C.⁵,Lin R. P.⁵,Elliott H.⁴

Affiliation:

1. LESIA and CNRS; Observatoire de Paris-Meudon; Meudon France

2. Department of Physics; West Virginia University; Morgantown West Virginia USA

3. Max-Planck-Institut für Sonnensystemforschung; Katlenburg-Lindau Germany

4. Space Science and Engineering Division; Southwest Research Institute; San Antonio Texas USA

5. Space Sciences Laboratory; University of California; Berkeley California USA

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference32 articles.

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3. Electron heat flow in the solar corona: Implications of non-Maxwellian velocity distributions, the solar gravitational field, and Coulomb collisions;Dorelli;J. Geophys. Res.,2003

4. Reconciling Spectroscopic electron temperature measurements in the solar corona with in situ charge state observations;Esser;Astrophys. J.,2000

5. Solar wind electrons;Feldman;J. Geophys. Res.,1975

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