Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Phil D Nicholson"'
Autor:
Valerio Poggiali, Giancorrado Brighi, Alexander G. Hayes, Phil D. Nicholson, Shannon MacKenzie, Daniel E. Lalich, Léa E. Bonnefoy, Kamal Oudrhiri, Ralph D. Lorenz, Jason M. Soderblom, Paolo Tortora, Marco Zannoni
Publikováno v:
Nature Communications, Vol 15, Iss 1, Pp 1-10 (2024)
Abstract Saturn’s moon Titan was explored by the Cassini spacecraft from 2004 to 2017. While Cassini revealed a lot about this Earth-like world, its radar observations could only provide limited information about Titan’s liquid hydrocarbons seas
Externí odkaz:
https://doaj.org/article/82c52dbcbf05419f99eb6bcc9e089f05
Autor:
Giancorrado Brighi, Valerio Poggiali, Paolo Tortora, Marco Zannoni, Alexander Hayes, Daniel Lalich, Lea Bonnefoy, Shannon MacKenzie, Phil D Nicholson, Kamal Oudrhiri, Ralph D Lorenz, Jason M Soderblom
Between 2006 and 2016, the Cassini spacecraft carried out 13 bistatic radar observations of the surface of Saturn's largest moon, Titan. Unmodulated right circularly polarized radio signals were transmitted by the spacecraft to the moon’s surface.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::52601164e710ef4d740b28e9847df2c8
https://doi.org/10.5194/egusphere-egu23-10075
https://doi.org/10.5194/egusphere-egu23-10075
Autor:
Sebastien Rodriguez, Bernd Giese, Robert H. Brown, T. Roatsch, Roland Wagner, Cristina M. Dalle Ore, Dale P. Cruikshank, Kevin H. Baines, Phil D. Nicholson, Dennis L. Matson, Roger N. Clark, Bonnie J. Buratti, Fabrizio Capaccioni, Ralf Jaumann, Norbert Krupp, Katrin Stephan, Gianrico Filacchione
Publikováno v:
Icarus
Icarus, 2016, 274, pp.1-22. ⟨10.1016/j.icarus.2016.03.002⟩
Icarus, 2016, 274, pp.1-22. ⟨10.1016/j.icarus.2016.03.002⟩
The Saturnian satellite Tethys exhibits geological and spectral properties, whose appearance, nature and spatial distribution partly mirror those identified on the neighboring satellites Dione and Rhea or fit to the picture how spectral surface prope
Autor:
Steve Miller, Emma J. Bunce, Bonnie J. Buratti, Robert H. Brown, Sarah V. Badman, Michele K. Dougherty, Christophe Sotin, Tom Stallard, Roger N. Clark, Chris S. Arridge, D. L. Talboys, Pierre Drossart, Phil D. Nicholson, Stan W. H. Cowley, Kevin H. Baines, Makenzie Lystrup, Nicholas Achilleos
Publikováno v:
Nature
Nature, 2008, 456, pp.214-217. ⟨10.1038/nature07440⟩
Nature, 2008, 456, pp.214-217. ⟨10.1038/nature07440⟩
Planetary aurorae are generally produced by currents flowing between the planet's ionosphere and magnetosphere, which accelerate energetic charged particles that then hit the upper atmosphere. Recent models of Saturn's aurora predict only weak emissi
Autor:
Jason W. Barnes, Sebastien Rodriguez, Bonnie J. Buratti, Stéphane Le Mouélic, Robert H. Brown, Kevin H. Baines, Laurence A. Soderblom, Roger N. Clark, Christophe Sotin, Phil D. Nicholson
Publikováno v:
Icarus. 186:242-258
We present global-scale maps of Titan from the Visual and Infrared Mapping Spectrometer (VIMS) instrument on Cassini. We map at 64 near-infrared wavelengths simultaneously, covering the atmospheric windows at 0.94, 1.08, 1.28, 1.6, 2.0, 2.8, and 5 μ
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 67:111-130
We study the rotational evolution under tidal torques of axisymmetric natural satellites in inclined, precessing orbits. In the spin- and orbit-averaged equations of motion, we find that a global limit cycle exists for parameter values near the stabi
The Canada–France ecliptic plane survey—full data release : the orbital structure of the Kuiper Belt
Autor:
Olivier Mousis, Jean-Marc Petit, Brian G. Marsden, Allyson Bieryla, Philippe Rousselot, Paula Gabriela Benavídez, Gilbert Mars, Matthew J. Taylor, Matthew L.N. Ashby, Joel Wm. Parker, Guillermo Bernabeu, Adriano Campo Bagatin, Christa Van Laerhoven, Brett Gladman, R. Lynne Jones, Phil D. Nicholson, Jj Kavelaars
Publikováno v:
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2011, 142 (4), pp.131. ⟨10.1088/0004-6256/142/4/131⟩
The Astronomical Journal, American Astronomical Society, 2011, 142 (131), ⟨10.1088/0004-6256/142/4/131⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
The Astronomical Journal, American Astronomical Society, 2011, 142 (4), pp.131. ⟨10.1088/0004-6256/142/4/131⟩
The Astronomical Journal, American Astronomical Society, 2011, 142 (131), ⟨10.1088/0004-6256/142/4/131⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
We report the orbital distribution of the trans-neptunian objects (TNOs) discovered during the Canada-France Ecliptic Plane Survey, whose discovery phase ran from early 2003 until early 2007. The follow-up observations started just after the first di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c13ecb983c41f123d58beddea122ed28
https://nrc-publications.canada.ca/eng/view/object/?id=52fd9c9a-9cf9-4469-8bab-b0ca257bd6ac
https://nrc-publications.canada.ca/eng/view/object/?id=52fd9c9a-9cf9-4469-8bab-b0ca257bd6ac
Autor:
Robert M. Nelson, Kevin H. Baines, Robert H. Brown, Klaus Dieter Matz, Dennis L. Matson, R. N. Clark, Thomas Roatsch, Katrin Stephan, Bernd Giese, Ralf Jaumann, Fabrizio Cappacioni, Charles A. Hibbitts, Gianrico Filacchione, F. Scholten, Dale P. Cruikshank, Phil D. Nicholson, Gary B. Hansen, Roland Wagner, Bonnie J. Buratti
Since the arrival of the Cassini spacecraft at Saturn in June 2004, the Visual and Infrared Mapping Spectrometer has obtained new spectral data of the icy satellites of Saturn in the spectral range from 0.35 to 5.2 μm. Numerous flybys were performed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a79c4bc8249c3e1e4352af44a9a586b7
https://elib.dlr.de/72695/
https://elib.dlr.de/72695/
Autor:
Phil D. Nicholson, Jason W. Barnes, Christophe Sotin, Stéphane Le Mouélic, Robert H. Brown, Roger N. Clark, Bonnie J. Buratti, Saïd Moussaoui, Pascal Rannou, Frédéric Schmidt, Sebastien Rodriguez, Kevin H. Baines
Publikováno v:
WHISPERS
Titan is the Saturn's largest moon where meteorological processes are very active, as observed most recently by the Cassini/Huygens orbiter. Cloud monitoring is a prime method to observe, describe and understand present climate on Titan. Unlike our p
Autor:
Robert H. Brown, G. Filiacchione, Charles A. Hibbitts, Ralf Jaumann, Harald Hoffmann, Gary B. Hansen, Thomas Roatsch, Roland Wagner, Dale P. Cruikshank, Bonnie J. Buratti, T. B. McCord, Katrin Stephan, Phil D. Nicholson, Kevin H. Baines, Roger N. Clark
We present a detailed analysis of the variations in spectral properties across the surface of Saturn’s satellite Dione using Cassini/VIMS data and their relationships to geological and/or morphological characteristics as seen in the Cassini/ISS ima
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4cbd8b9a1fb069dcc08173a8205d5df
https://elib.dlr.de/61126/
https://elib.dlr.de/61126/