Why the 46° halo is seen far less often than the 22° halo? - Université Clermont Auvergne Accéder directement au contenu
Article Dans Une Revue Journal of Quantitative Spectroscopy and Radiative Transfer Année : 2013

Why the 46° halo is seen far less often than the 22° halo?

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hal-01823405 , version 1 (26-06-2018)

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Valery Shcherbakov. Why the 46° halo is seen far less often than the 22° halo?. Journal of Quantitative Spectroscopy and Radiative Transfer, 2013, 124, pp.37 - 44. ⟨10.1016/j.jqsrt.2013.03.002⟩. ⟨hal-01823405⟩
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