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Knollenberg, J.-L. Bertaux, J.-R. Kramm, L. Jorda, L. M. Lara, M. A. Barucci, M. De Cecco, M. F. A'Hearn, M. Fulle, M. Hofmann, M. Kueppers, M. Lazzarin, M. Massironi, M. Pajola, M. R. El-Maarry, N. Masoumzadeh, N. Oklay, N. Thomas, O. Groussin, P. Gutierrez-Marquez, P. J. Gutierrez, P. L. Lamy, R. Rodrigo, S. Besse, S. Debei, S. F. Hviid, S. Fornasier, S. Hoefner, S. Lowry, S. Mottola, V. Da Deppo, W.-H. Ip, X. Hu, X. Shi, Z.-Y. Lin","submitted_at":"2016-08-31T09:04:56Z","abstract_excerpt":"Beginning in March 2014, the OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) cameras began capturing images of the nucleus and coma (gas and dust) of comet 67P/Churyumov-Gerasimenko using both the wide angle camera (WAC) and the narrow angle camera (NAC). The many observations taken since July of 2014 have been used to study the morphology, location, and temporal variation of the comet's dust jets. 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