Production of non-gyrotropic and gyrotropic backstreaming ion distributions in the quasi-perpendicular ion foreshock region : Origin and acceleration mechanisms.

Philippe Savoini; Bertrand Lembège

Poster communications

Production of non-gyrotropic and gyrotropic backstreaming ion distributions in the quasi-perpendicular ion foreshock region : Origin and acceleration mechanisms.

Philippe Savoini ¹ Bertrand Lembège ²

1 LPP - Laboratoire de Physique des Plasmas

2 HELIOS - LATMOS

LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales

Document type :

Poster communications

Domain :

Sciences of the Universe [physics] / Astrophysics [astro-ph] / Earth and Planetary Astrophysics [astro-ph.EP]

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https://hal-insu.archives-ouvertes.fr/insu-01142775
Contributor : Catherine Cardon <>
Submitted on : Wednesday, April 15, 2015 - 8:33:12 PM
Last modification on : Wednesday, April 14, 2021 - 3:39:46 AM

Production of non-gyrotropic and gyrotropic backstreaming ion distributions in the quasi-perpendicular ion foreshock region : Origin and acceleration mechanisms.

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Production of non-gyrotropic and gyrotropic backstreaming ion distributions in the quasi-perpendicular ion foreshock region : Origin and acceleration mechanisms.

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