Diurnal variation of dust and gas production in comet 67P/Churyumov-Gerasimenko at the inbound equinox as seen by OSIRIS and VIRTIS-M on board Rosetta

<strong>Context.</strong> On 27 April 2015, when comet 67P/Churyumov-Gerasimenko was at 1.76 au from the Sun and moving toward perihelion, the OSIRIS and VIRTIS-M instruments on board the Rosetta spacecraft simultaneously observed the evolving dust and gas coma during a complete rotation...

詳細記述

書誌詳細
主要な著者: Tubiana, C, Rinaldi, G, Guettler, C, Taylor, F, Et al.
フォーマット: Journal article
言語:English
出版事項: EDP Sciences 2019