Dual Maxwellian-Kappa modelling of the solar wind electrons: new clues on the temperature of Kappa populations

Lazar, M.; Pierrard, Viviane; Shaaban, S.M.; Fichtner, H.; Poedts, S.

doi:10.1051/0004-6361/201630194

Dual Maxwellian-Kappa modelling of the solar wind electrons: new clues on the temperature of Kappa populations

Lazar, M.

;

Pierrard, Viviane

;

Shaaban, S.M.

;

Fichtner, H.

;

Poedts, S.

(2017) Astronomy & Astrophysics — Vol. A44, p. 10 p. (2017)

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Authors

Lazar, M.Centre for Mathematical Plasma Astrophysics, Celestijnenlaan 200B, 3001 Leuven, Belgium
Author
Pierrard, VivianeUCLouvain
Author
Shaaban, S.M.Centre for Mathematical Plasma Astrophysics, Celestijnenlaan 200B, 3001 Leuven, Belgium
Author
Fichtner, H.Institut für Theoretische Physik, Lehrstuhl IV: Weltraum- und Astrophysik, Ruhr-Universität Bochum, 44780 Bochum, Germany
Author
Poedts, S.Centre for Mathematical Plasma Astrophysics, Celestijnenlaan 200B, 3001 Leuven, Belgium
Author

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UCLouvainSST/ELI/ELIC - Earth & Climate

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Lazar, M., Pierrard, V., Shaaban, S. M., Fichtner, H., & Poedts, S. (2017). Dual Maxwellian-Kappa modelling of the solar wind electrons: new clues on the temperature of Kappa populations. Astronomy & Astrophysics, A44, 10 p. https://doi.org/10.1051/0004-6361/201630194 (Original work published 2017)