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
C. Tubiana, G. Rinaldi, C. Güttler, C. Snodgrass, X. Shi, X. Hu, R. Marschall, M. Fulle, D. Bockelée-Morvan, G. Naletto, F. Capaccioni, H. Sierks, G. Arnold, M. A. Barucci, J. -L. Bertaux, I. Bertini, D. Bodewits, M. T. Capria, M. Ciarniello, G. CremoneseJ. Crovisier, V. Da Deppo, S. Debei, M. De Cecco, J. Deller, M. C. De Sanctis, B. Davidsson, L. Doose, S. Erard, G. Filacchione, U. Fink, M. Formisano, S. Fornasier, P. J. Gutiérrez, W. -H. Ip, S. Ivanovski, D. Kappel, H. U. Keller, L. Kolokolova, D. Koschny, H. Krueger, F. La Forgia, P. L. Lamy, L. M. Lara, M. Lazzarin, A. C. Levasseur-Regourd, Z. -Y. Lin, A. Longobardo, J. J. López-Moreno, F. Marzari, A. Migliorini, S. Mottola, R. Rodrigo, F. Taylor, I. Toth, V. Zakharov
Research output: Contribution to journal › Article › peer-review
Fingerprint
Dive into the research topics of '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'. Together they form a unique fingerprint.