Radial evolution of nonthermal electron populations in the low-latitude solar wind: Helios, Cluster, and Ulysses Observations

Author:

Štverák Štěpán12,Maksimovic Milan2,Trávníček Pavel M.13,Marsch Eckart4,Fazakerley Andrew N.5,Scime Earl E.6

Affiliation:

1. Department of Space Physics, Institute of Atmospheric Physics; Academy of Sciences of the Czech Republic; Prague Czech Republic

2. LESIA, Observatoire de Paris, CNRS, UPMC; Université Paris Diderot; Meudon France

3. Astronomical Institute; Academy of Sciences of the Czech Republic; Prague Czech Republic

4. Department for Sun and Heliosphere; Max Planck Institute for Solar System Research; Katlenburg-Lindau Germany

5. Mullard Space Science Laboratory; University College London; Dorking UK

6. Department of Physics; West Virginia University; Morgantown West Virginia 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

Reference48 articles.

1. The Ulysses solar wind plasma experiment;Bame;Astron. Astrophys. Suppl. Ser.,1992

2. Large-scale magnetic field inversions at sector boundaries;Crooker;J. Geophys. Res.,2004

3. Cluster: Science and mission overview;Escoubet;Space Sci. Rev.,1997

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

5. Electron density and temperature of the lower solar corona;Fludra;J. Geophys. Res.,1999

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