The Electron Temperature and Anisotropy in the Solar Wind. Comparison of the Core and Halo Populations
Author:
Funder
Belgian Federal Policy (BE)
FWO-Vlaanderen
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-016-0961-7.pdf
Reference38 articles.
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3. Collier, M.R., Hamilton, D.C., Gloeckler, G., Bochsler, P., Sheldon, R.B.: 1996, Neon-20, Oxigen-16, and Helium-4 densities, temperatures, and suprathermal tails in the solar wind determined with WIND/MASS. Geophys. Res. Lett. 23, 1191. DOI .
4. Feldman, W.C., Asbridge, J.R., Bame, S.J., Montgomery, M.D., Gary, S.P.: 1975, Solar wind electrons. J. Geophys. Res. 80, 4181. DOI .
5. Gary, S.P., Saito, S.: 2007, Broadening of solar wind strahl pitch-angles by the electron/electron instability: Particle-in-cell simulations. Geophys. Res. Lett. 34, L14111. DOI .
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