Zobrazeno 1 - 10
of 18
pro vyhledávání: '"G. Francescetti"'
Autor:
G. Boubin, Michael Allison, Ellen R. Stofan, Charles Elachi, G. Hamilton, Steven J. Ostro, L. Roth, Randolph L. Kirk, William T. K. Johnson, Stephen D. Wall, Y. Anderson, S. Shaffer, Roberto Seu, Philip S. Callahan, Lauren Wye, R. Boehmer, Bryan Stiles, Gian Gabriele Ori, Jani Radebaugh, Karl L. Mitchell, Giovanni Picardi, Howard A. Zebker, Laurence A. Soderblom, Duane O. Muhleman, Richard West, S. Vetrella, Enrico Flamini, R. D. Lorenz, Roberto Orosei, Andrew Dominic Fortes, Jonathan I. Lunine, Yonggyu Gim, K. Kelleher, L. E. Robshaw, Catherine D. Neish, E. Reffet, Pierre Encrenaz, Scott Hensley, Flora Paganelli, Michael Janssen, Rosaly M. C. Lopes, Francesco Posa, Charles A. Wood, G. Francescetti
Publikováno v:
Icarus
Icarus, 2007, 186, pp.395-412. ⟨10.1016/j.icarus.2006.09.006⟩
Icarus, 2007, 186, pp.395-412. ⟨10.1016/j.icarus.2006.09.006⟩
International audience; The Cassini Titan Radar Mapper obtained Synthetic Aperture Radar images of Titan's surface during four fly-bys during the mission's first year. These images show that Titan's surface is very complex geologically, showing evide
Autor:
Howard A. Zebker, L. Roth, Ralph D. Lorenz, Bryan Stiles, Charles Elachi, Y. Anderson, Ellen R. Stofan, Roberto Seu, K. Kelleher, Giovanni Picardi, Gian Gabriele Ori, K. L. Mitchell, E. Reffet, Duane O. Muhleman, Jonathan I. Lunine, Jani Radebaugh, Enrico Flamini, G. Boubin, Yonggyu Gim, Lauren Wye, S. D. Wall, G. Francescetti, Robert West, Matthew A. Allison, S. Vetrella, Rosaly M. C. Lopes, G. Hamilton, Philip S. Callahan, Laurence A. Soderblom, R. Boehmer, S. Shaffer, Steven J. Ostro, Randolph L. Kirk, Pierre Encrenaz, Scott Hensley, M. A. Janssen, Flora Paganelli, William L. Johnson, Francesco Posa, Charles A. Wood
Publikováno v:
Science
Science, 2006, 312, pp.724-727. ⟨10.1126/science.1123257⟩
Science, 2006, 312, pp.724-727. ⟨10.1126/science.1123257⟩
The most recent Cassini RADAR images of Titan show widespread regions (up to 1500 kilometers by 200 kilometers) of near-parallel radar-dark linear features that appear to be seas of longitudinal dunes similar to those seen in the Namib desert on Eart
Autor:
C. Elachi, S. Wall, M. Allison, Y. Anderson, R. Boehmer, P. Callahan, P. Encrenaz, E. Flamini, G. Francescetti, Y. Gim, G. Hamilton, S. Hensley, M. Janssen, W. Johnson, K. Kelleher, R. Kirk, R. Lopes, R. Lorenz, J. Lunine, D. Muhleman, S. Ostro, F. Paganelli, G. Picardi, F. Posa, L. Roth, R. Seu, S. Shaffer, L. Soderblom, B. Stiles, E. Stofan, R. West, C. Wood, L. Wye, H. Zebker, VETRELLA, SERGIO
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3730::5d2bf6cb0c04b24464de40f893cbbca1
http://hdl.handle.net/11588/414314
http://hdl.handle.net/11588/414314
Autor:
Pierre Encrenaz, S. Hensley, G. Hamilton, Steven J. Ostro, Randolph L. Kirk, Michael Janssen, Rosaly M. C. Lopes, Philip S. Callahan, Yonggyu Gim, Roberto Seu, E. Flamini, R. D. Lorenz, K. Kelleher, Giovanni Picardi, Duane O. Muhleman, L. Roth, Matthew A. Allison, Y. Anderson, Howard A. Zebker, William T. K. Johnson, Jani Radebaugh, Francesco Posa, Laurence A. Soderblom, Charles A. Wood, Lauren Wye, Bryan Stiles, Jonathan I. Lunine, R. Boehmer, G. Francescetti, S. Shaffer, P. Paillou, Charles Elachi, Karl L. Mitchell, Flora Paganelli, Robert West, S. Vetrella, Ellen R. Stofan, S. D. Wall
Publikováno v:
Nature
Nature, Nature Publishing Group, 2007, 445 (7123), pp.61-64. ⟨10.1038/nature05438⟩
Nature, Nature Publishing Group, 2007, 445 (7123), pp.61-64. ⟨10.1038/nature05438⟩
The surface of Saturn's haze-shrouded moon Titan has long been proposed to have oceans or lakes, on the basis of the stability of liquid methane at the surface1, 2. Initial visible3 and radar4, 5 imaging failed to find any evidence of an ocean, altho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::625560c4c1c6f9eb4690c57191842d16
https://hal.archives-ouvertes.fr/hal-00159750
https://hal.archives-ouvertes.fr/hal-00159750
Autor:
Pierre Encrenaz, Scott Hensley, William L. Johnson, Ellen R. Stofan, Roberto Seu, R. Boehmer, Steven J. Ostro, Randolph L. Kirk, Rosaly M. C. Lopes, K. Kelleher, Flora Paganelli, Matthew A. Allison, S. Vetrella, E. Flamini, Francesco Posa, G. Francescetti, G. Hamilton, Robert West, Laurence A. Soderblom, Charles A. Wood, Philip S. Callahan, Ralph D. Lorenz, Charles Elachi, S. D. Wall, S. Shaffer, Howard A. Zebker, M. A. Janssen, Bryan Stiles, Yonggyu Gim, L. Roth, Y. Anderson, Giovanni Picardi, Duane O. Muhleman, Jonathan I. Lunine, Lauren Wye
Publikováno v:
Nature
Nature, 2006, 441, pp.709-713. ⟨10.1038/nature04786⟩
Nature, 2006, 441, pp.709-713. ⟨10.1038/nature04786⟩
International audience; Cassini's Titan Radar Mapper imaged the surface of Saturn's moon Titan on its February 2005 fly-by (denoted T3), collecting high-resolution synthetic-aperture radar and larger-scale radiometry and scatterometry data. These dat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10c7a702520e79eb331c2dc5ec64c2f8
http://hdl.handle.net/11588/329012
http://hdl.handle.net/11588/329012
Autor:
Flora Paganelli, R. Boehmer, Philip S. Callahan, Matthew A. Allison, S. Shaffer, Yonggyu Gim, M. A. Janssen, Enrico Flamini, Robert West, G. Hamilton, Pierre Encrenaz, Ralph D. Lorenz, Rosaly M. C. Lopes, Laurence A. Soderblom, Scott Hensley, Howard A. Zebker, Charles Elachi, Giovanni Picardi, K. Kelleher, Duane O. Muhleman, William T. K. Johnson, Francesco Posa, Charles A. Wood, G. Francescetti, Jonathan I. Lunine, Lauren Wye, L. Roth, Y. Anderson, Bryan Stiles, Ellen R. Stofan, Steven J. Ostro, Randolph L. Kirk, S. D. Wall, S. Vetrella, Roberto Seu, Jani Radebaugh
The first two swaths collected by Cassini's Titan Radar Mapper were obtained in October of 2004 (Ta) and February of 2005 (T3). The Ta swath provides evidence for cryovolcanic processes, the possible occurrence of fluvial channels and lakes, and some
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8c6b83335d8944c122e81860612c0c09
http://hdl.handle.net/11573/69685
http://hdl.handle.net/11573/69685
Autor:
Howard A. Zebker, Pierre Encrenaz, S. Hensley, L. A. Soderblom, L. Roth, Steven J. Ostro, Rosaly M. C. Lopes, Ellen R. Stofan, Enrico Flamini, Matthew A. Allison, Charles Elachi, Y. Anderson, G. Francescetti, S. Vetrella, M. A. Janssen, R. D. Lorenz, Roberto Seu, R. Boehmer, Flora Paganelli, William L. Johnson, R. L. Kirk, Philip S. Callahan, Jonathan I. Lunine, S. Shaffer, Bryan Stiles, Francesco Posa, Charles A. Wood, S. D. Wall, Giovanni Picardi, K. Kelleher, G. Hamilton, Duane O. Muhleman, Lauren Wye, Yonggyu Gim, Robert West
Publikováno v:
Nature. 442:594-594
Nature 441, 709–713 (2006) In this Article, Fig. 2 was printed in reverse (bright areas appeared dark and vice versa). The correct figure is reprinted below.
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