Electron temperature anisotropy constraints in the solar wind

By Š. Štverák, P. Trávnícek, M. Maksimović, Eckart Marsch, A. Fazakerley, E. Scime. 2008

208 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/2958b5c9f1060bdcc206e9638f1e27025919eb0d

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Citations in the corpus

• Radial evolution of nonthermal electron populations in the low‐latitude solar wind: Helios, Cluster, and Ulysses Observations (2009, unknown): “the core population is concerned, Štverák et al. [2008] presented clear observational evidence that both collision and wave-particle interactions are effective in constraining”
• Kappa Distributions: Theory and Applications in Space Plasmas (2010, background): “…a result of low collision rates in the interplanetary plasm , the electrons and the ions develop temperature anisotropies and their VDFs become skewed and develop tails and heat fluxes along the ambient magnetic field (Marsch et al. 1982; Pilipp et al. 1987; Salem et al. 2003; Stverak et al. 2008).”