Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Rebecca A. Harbison"'
Autor:
Kate Craft, Roland M. B. Young, Paolo Tortora, Ravit Helled, Jonathan J. Fortney, Robert Ebert, Wes Patterson, S. Luszcz-Cook, Alice Lucchetti, Carol Paty, C. M. Jackman, Alessandro Mura, Alan Stern, Alice Cocoros, Ian J. Cohen, Chloe B. Beddingfield, Katrin Stephan, Jesper Gjerloev, Lynnae C. Quick, Catherine Elder, Robert A. Dillman, Drew Turner, Peter Wurz, Matina Gkioulidou, Shawn Brueshaber, Chris Paranicas, Kunio M. Sayanagi, Sasha Ukhorskiy, Sarah E. Moran, R. Nikoukar, Kirby Runyon, Michael H. Wong, Todd Smith, Carolyn M. Ernst, Maurizio Pajola, Matthew M. Hedman, Gianrico Filacchione, Yasumasa Kasaba, Marzia Parisi, Leigh N. Fletcher, Chuanfei Dong, Caitlin Ahrens, Gina A. DiBraccio, Shawn Brooks, Robert Chancia, Michael P. Lucas, Leonardo Regoli, Imke de Pater, Alena Probst, Peter Kollmann, Athena Coustenis, James H. Roberts, Daniel J. Gershman, Lauren Jozwiak, Soumyo Dutta, Linda Spilker, Elizabeth P. Turtle, Sebastien Rodriguez, Yongliang Zhang, Gangkai Poh, George Clark, Tibor S. Balint, Ingrid Daubar, Kathleen Mandt, Adam Masters, Richard Holme, Devanshu Jha, Go Murakami, Noemi Pinilla-Alonso, Sarah K. Vines, Olivier Mousis, Krista M. Soderlund, Athul Pradeepkumar Girija, Ronald J. Vervack, Corey J. Cochrane, Xin Cao, Emma J. Bunce, Shannon MacKenzie, George Hospodarsky, Sébastien Charnoz, Elena Adams, Kimberly Moore, Erin Leonard, Heather Meyer, Rebecca A. Harbison, Abigail Rymer, Sabine Stanley, Barry Mauk, Richard Cartwright
Publikováno v:
Bulletin of the AAS. 53
Autor:
Roger N. Clark, Kevin H. Baines, Christophe Sotin, Todd M. Ansty, Rebecca A. Harbison, Philip D. Nicholson, Robert H. Brown, Douglas Creel, Johnathon Ahlers, Bonnie J. Buratti, Sarah V. Badman, Matthew M. Hedman
We describe the prediction, design, execution and calibration of stellar and solar occultation observations of Saturn's rings by the Visual and Infrared Mapping Spectrometer (VIMS) instrument on the Cassini spacecraft. Particular attention is paid to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7bb9b23710ca9e9c80b7fa526a2d95e5
https://doi.org/10.1016/j.icarus.2019.06.017
https://doi.org/10.1016/j.icarus.2019.06.017
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 110:1-16
Saturn’s moon, Hyperion, is subject to strongly-varying solid body torques from its primary and lacks a stable spin state resonant with its orbital frequency. In fact, its rotation is chaotic, with a Lyapunov timescale on the order of 100 days. In
Radio occultations of Saturn's main rings by spacecraft suggest a power law particle size-distribution down to sizes of the order of 1 cm (Marouf et al., 1983), (Zebker et al., 1985). The lack of optical depth variations between ultraviolet and near-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2ce53a15090b5ea8675e4a3257932f5
http://arxiv.org/abs/1312.2927
http://arxiv.org/abs/1312.2927