Non-thermal velocity distribution functions in the interplanetary medium : on their origin and consequences for the Solar Wind acceleration - Archive ouverte HAL Accéder directement au contenu
Communication Dans Un Congrès Année : 2004

Non-thermal velocity distribution functions in the interplanetary medium : on their origin and consequences for the Solar Wind acceleration

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hal-03724379 , version 1 (15-07-2022)

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  • HAL Id : hal-03724379 , version 1

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Milan Maksimovic. Non-thermal velocity distribution functions in the interplanetary medium : on their origin and consequences for the Solar Wind acceleration. Alfvén 2004 Workshop on Space Environment Turbulence, 2004, Beaulieu, France, France. ⟨hal-03724379⟩
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