On the existence of non-Maxwellian velocity distribution functions in the corona and their consequences for the Solar Wind acceleration - Archive ouverte HAL Accéder directement au contenu
Communication Dans Un Congrès Année : 2004

On the existence of non-Maxwellian velocity distribution functions in the corona and their consequences for the Solar Wind acceleration

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hal-03724361 , version 1 (15-07-2022)

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  • HAL Id : hal-03724361 , version 1

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Milan Maksimovic. On the existence of non-Maxwellian velocity distribution functions in the corona and their consequences for the Solar Wind acceleration. CESRA Workshop on, 2004, Sabhal Mor Ostaig, Isle of Skye, United Kingdom. ⟨hal-03724361⟩
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