Spectral properties of icy saturnian satellites derived from cassini data
暂无分享,去创建一个
Robert H. Brown | Roland Wagner | Bonnie J. Buratti | Kevin H. Baines | Ralf Jaumann | Dale P. Cruikshank | Gianrico Filacchione | Thomas Roatsch | Roger N. Clark | Katrin Stephan | Phil D. Nicholson | Cristina Dalle Ore | Bernd Giese | Dennis Matson | Fabrizio Cappacione | R. Clark | R. Jaumann | B. Buratti | K. Baines | D. Matson | T. Roatsch | G. Filacchione | K. Stephan | B. Giese | D. Cruikshank | R. Wagner | P. Nicholson | C. Ore | Robert H. Brown | Fabrizio Cappacione | R. Clark
[1] T. Owen,et al. A spectroscopic study of the surfaces of Saturn's large satellites: H 2 O ice, tholins, and minor constituents , 2005 .
[2] J. Veverka,et al. Voyager photometry of Rhea, Dione, Tethys, Enceladus and Mimas , 1984 .
[3] R. Clark,et al. Compositional mapping of Saturn's satellite Dione with Cassini VIMS and implications of dark material in the Saturn system , 2007 .
[4] J. Burns,et al. Cassini Imaging Science: Instrument Characteristics And Anticipated Scientific Investigations At Saturn , 2004 .
[5] M. Showalter,et al. Plasma, plumes and rings: Saturn system dynamics as recorded in global color patterns on its midsize icy satellites , 2011 .
[6] R. H. Brown,et al. The Cassini Visual And Infrared Mapping Spectrometer (Vims) Investigation , 2004 .
[7] R. Clark,et al. Dione's spectral and geological properties , 2010 .