Non-thermal velocity distribution functions in the interplanetary medium : on their origin and consequences for the Solar Wind acceleration - Archive ouverte HAL
Communication Dans Un Congrès Année : 2003

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

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hal-03729686 , version 1 (20-07-2022)

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  • HAL Id : hal-03729686 , 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. 4th Serbian Conference on Spectral Lines Shapes (IV SCSLS), 2003, Arandelovac, Serbie Monténégro, Serbia. ⟨hal-03729686⟩
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