Observations of the hydrogen corona of Venus by SPICAV/Vénus Express
Résumé
Observations of the H corona before Vénus Express. Diurnal variations derived by PVO. Formation of the hydrogen corona. SPICAV-UV/VEX. Lyman--alpha emission. Forward approach for dayside observations. ObservaEons at the dayside and observaEons at the nightside. Forward approach for shadow observaEons
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