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A New 3D Multi-fluid Dust Model: A Study of the Effects of Activity and Nucleus Rotation on Dust Grain Behavior at Comet 67P/Churyumov–Gerasimenko

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Ionospheric plasma of comet 67P probed byRosettaat 3 au from the Sun

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Analysis of the dust jet imaged byRosettaVIRTIS-M in the coma of comet 67P/Churyumov–Gerasimenko on 2015 April 12

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Seasonal exposure of carbon dioxide ice on the nucleus of comet 67P/Churyumov-Gerasimenko

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Rosetta’s comet 67P/Churyumov-Gerasimenko sheds its dusty mantle to reveal its icy nature

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2D photochemical model for forbidden oxygen line emission for comet 1P/Halley

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67P/C-G inner coma dust properties from 2.2 au inbound to 2.0 au outbound to the Sun

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Observations of high-plasma density region in the inner coma of 67P/Churyumov–Gerasimenko during early activity

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https://doi.org/10.1093/mnras/stw1663

CHANGES IN THE PHYSICAL ENVIRONMENT OF THE INNER COMA OF 67P/CHURYUMOV–GERASIMENKO WITH DECREASING HELIOCENTRIC DISTANCE

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The Astronomical Journal 152 (5) 130 (2016)
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Evolution of CO2, CH4, and OCS abundances relative to H2O in the coma of comet 67P around perihelion fromRosetta/VIRTIS-H observations

Dominique Bockelée-Morvan, J. Crovisier, S. Erard, et al.
Monthly Notices of the Royal Astronomical Society 462 (Suppl 1) S170 (2016)
https://doi.org/10.1093/mnras/stw2428

Structure and evolution of the diamagnetic cavity at comet 67P/Churyumov–Gerasimenko

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Monthly Notices of the Royal Astronomical Society 462 (Suppl 1) S459 (2016)
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