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Akademický článek
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INTRODUCTION Our view of planetary ring particles and the characteristics of their thermal emission has undergone a major paradigm shift since the arrival of Cassini at Saturn. Our understanding of the microstructure and microphysics of the rings has
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b1116394eb36637a7ef3b1647831e313
https://doi.org/10.1017/9781316286791.015
https://doi.org/10.1017/9781316286791.015
Autor:
David Lopez-Paz, S. G. Edgington, Alberto Flandes, Shawn M. Brooks, E. Deau, R. Morishima, Nicolas Altobelli, Linda Spilker, S. Pilorz, C. Leyrat
Publikováno v:
Icarus
Icarus, Elsevier, 2014, 238, pp.205-220. ⟨10.1016/j.icarus.2014.04.031⟩
Icarus, Elsevier, 2014, 238, pp.205-220. ⟨10.1016/j.icarus.2014.04.031⟩
We present two numerical models designed to reproduce the temperatures of the illuminated Saturn rings as measured by the CASSINI-CIRS instrument. Our models are constrained by all available temperature measurements performed on the illuminated rings
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc1e3588c57a7cc4d8ff70c9b0327fa8
https://doi.org/10.1016/j.icarus.2014.04.031
https://doi.org/10.1016/j.icarus.2014.04.031
Autor:
Gordon L. Bjoraker, John C. Pearl, Daniel Gautier, Tobias Owen, R. K. Achterberg, Nicholas A Teanby, S. B. Calcutt, V. G. Kunde, Athena Coustenis, C. Ferrari, Mark R. Showalter, Antonella Barucci, Neil Bowles, E. H. Wishnow, Patrick G. J. Irwin, B. Wallis, Linda Spilker, Regis Courtin, John R. Spencer, Scott G. Edgington, F. M. Flasar, Conor A. Nixon, M. E. Segura, Peter L. Read, Amy A. Simon-Miller, Thierry Fouchet, S. Pilorz, Bruno Bézard, Paul N. Romani, A. A. Mamoutkine, Paul J. Schinder, Emmanuel Lellouch, Robert E. Samuelson, Barney J. Conrath, Ronald Carlson, Peter J. Gierasch, Mian M. Abbas, John C. Brasunas, François Raulin, R. Prangé, Fredric W. Taylor, Glenn S. Orton, D. E. Jennings, Darrell F. Strobel, A. Marten, Peter A. R. Ade
Publikováno v:
Science
Science, American Association for the Advancement of Science (AAAS), 2005, 307, pp.1247-1251. ⟨10.1126/science.1105806⟩
Science, 2005, 307, pp.1247-1251. ⟨10.1126/science.1105806⟩
Science, American Association for the Advancement of Science (AAAS), 2005, 307, pp.1247-1251. ⟨10.1126/science.1105806⟩
Science, 2005, 307, pp.1247-1251. ⟨10.1126/science.1105806⟩
International audience; Stratospheric temperatures on Saturn imply a strong decay of the equatorial winds with altitude. If the decrease in winds reported from recent Hubble Space Telescope images is not a temporal change, then the features tracked m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a233a114517cf76158eca7d61ea99131
https://doi.org/10.1126/science.1105806
https://doi.org/10.1126/science.1105806
Publikováno v:
Planetary and Space Science. 56:134-146
Two and a half years after Saturn orbit insertion (SOI) the Cassini composite infrared spectrometer (CIRS) has acquired an extensive set of thermal measurements (including physical temperature and filling factor) of Saturn's main rings for a number o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::47f0e3fa79455ddb82a81eb167f2a6f2
https://doi.org/10.1016/j.pss.2007.05.029
https://doi.org/10.1016/j.pss.2007.05.029
Autor:
Shawn M. Brooks, S. Pilorz, B. Wallis, Linda Spilker, M. Flasar, Nicolas Altobelli, S. G. Edgington
Publikováno v:
Icarus. 191:691-701
We analyze data sets obtained with the Composite Infrared Spectrometer (CIRS) onboard the Cassini spacecraft after the Saturn Orbit Insertion (SOI). Using the mid-IR interferometer's FP3 channel (600–1100 cm −1 ), we derive radial temperature pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8dc8124e9dd0f35d1080879e52409f9b
https://doi.org/10.1016/j.icarus.2007.06.014
https://doi.org/10.1016/j.icarus.2007.06.014
Autor:
John C. Pearl, S. G. Edgington, S. Pilorz, Linda Spilker, B. Wallis, Shawn M. Brooks, F. M. Flasar
Publikováno v:
Earth, Moon, and Planets. 96:149-163
The Cassini Composite Infrared Spectrometer (CIRS) spatially resolved Saturn’s main rings in the far-infrared, measuring the spectrum from 20 to 400 wavenumbers (cm−1) (tens of microns to submillimeter wavelengths). We find a spectral roll-off be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8726b8228467e733cda5a05207bd4d5b
https://doi.org/10.1007/s11038-005-9060-8
https://doi.org/10.1007/s11038-005-9060-8
Autor:
Benjamin Pollard, Robert M. Nelson, Christopher T. Russell, S. Pilorz, Linda Spilker, Arthur L. Lane
Publikováno v:
Icarus. 171:372-390
We have undertaken an analysis of the Voyager photopolarimeter (PPS) stellar occultation data of Saturn's A ring. The Voyager PPS observed the bright star δ Scorpii as it was occulted by Saturn's main rings during the spacecraft flyby of the Saturn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9abe33159a87cb0fcf39b88c2d299fa8
https://doi.org/10.1016/j.icarus.2004.05.016
https://doi.org/10.1016/j.icarus.2004.05.016