Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Lauren Wye"'
Autor:
Travis Imken, Simone Tanelli, David Hawkins, Lauren Wye, Eva Peral, Jim Hoffman, Simon Lee, Stephen Horst, Sang-Ho Yun, Yahya Rahmat-Samii, Eastwood Im
Publikováno v:
Proceedings of the IEEE. 106:404-418
Space-based radar observations have transformed our understanding of Earth over the last several decades. Driven by increasingly complex science questions, space radar missions have grown ever more sophisticated with costs rising often to hundreds of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4cf3710901f893d52f0c5ede370de0aa
https://doi.org/10.1109/jproc.2018.2793179
https://doi.org/10.1109/jproc.2018.2793179
Autor:
M. A. Janssen, Howard A. Zebker, Alice Le Gall, Ralph D. Lorenz, Alexander G. Hayes, Lauren Wye
Publikováno v:
Geophysical Research Letters. 41:308-313
Cassini radar observations of the surface of Ligeia Mare collected during the 23 May 2013 (T91) Cassini fly-by show that it is extremely smooth, likely to be mostly methane in composition, and exhibits no surface wave activity. The radar parameters w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::84fe9e407e3af6d84a38381e3d2f1937
https://doi.org/10.1002/2013gl058877
https://doi.org/10.1002/2013gl058877
Autor:
Michael Malaska, S. D. Wall, Jeffrey S. Kargel, Ellen R. Stofan, Jonathan I. Lunine, Rosaly M. C. Lopes, Lauren Wye, M. A. Janssen, Jani Radebaugh, A. Legall, Jason W. Barnes, Catherine D. Neish, Karl L. Mitchell, Charles A. Wood, Alexander G. Hayes, Randolph L. Kirk
Publikováno v:
Journal of Geophysical Research: Planets. 118:416-435
[1] The existence of cryovolcanic features on Titan has been the subject of some controversy. Here we use observations from the Cassini RADAR, including Synthetic Aperture Radar (SAR) imaging, radiometry, and topographic data as well as compositional
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::655f341f5be8b71d156e2d4ffd888094
https://doi.org/10.1002/jgre.20062
https://doi.org/10.1002/jgre.20062
Autor:
Domenico Casarano, Francesco Posa, B. Ventura, Claudia Notarnicola, Lauren Wye, Alexander Hayes
Publikováno v:
Icarus (N.Y.N.Y. 1962) 221 (2012): 960–969. doi:10.1016/j.icarus.2012.09.011
info:cnr-pdr/source/autori:B. Ventura, C. Notarnicola, D. Casarano, F. Posa, A. G. Hayes, L. Wye/titolo:Electromagnetic models and inversion techniques for Titan's Ontario Lacus depth estimation from Cassini RADAR data/doi:10.1016%2Fj.icarus.2012.09.011/rivista:Icarus (N.Y.N.Y. 1962)/anno:2012/pagina_da:960/pagina_a:969/intervallo_pagine:960–969/volume:221
info:cnr-pdr/source/autori:B. Ventura, C. Notarnicola, D. Casarano, F. Posa, A. G. Hayes, L. Wye/titolo:Electromagnetic models and inversion techniques for Titan's Ontario Lacus depth estimation from Cassini RADAR data/doi:10.1016%2Fj.icarus.2012.09.011/rivista:Icarus (N.Y.N.Y. 1962)/anno:2012/pagina_da:960/pagina_a:969/intervallo_pagine:960–969/volume:221
Since 2004, Cassini RADAR, operating at 13.8 GHz as a radiometer, scatterometer, altimeter and synthetic aperture radar (SAR), provides a vast amount of data, suggesting new scenarios for Titan’s morphology and evolution. An important result was th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0707f8cb598d16a4f039981b21929721
https://doi.org/10.1016/j.icarus.2012.09.011
https://doi.org/10.1016/j.icarus.2012.09.011
Publikováno v:
Icarus. 212:321-328
Since Cassini arrived at Saturn in 2004, its moon Titan has been thoroughly mapped by the RADAR instrument at 2-cm wavelength, in both active and passive modes. Some regions on Titan, including Xanadu and various bright hummocky bright terrains, cont
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0c8f7b1ed7615ddfdee5e2bdd159d9f8
https://doi.org/10.1016/j.icarus.2010.11.026
https://doi.org/10.1016/j.icarus.2010.11.026
Autor:
S. D. Wall, Alexander G. Hayes, Ellen R. Stofan, Jonathan I. Lunine, Flora Paganelli, R. L. Kirk, Charles A. Wood, P. Valora, Rosaly M. C. Lopes, M. A. Janssen, A. Legall, Jani Radebaugh, Ralph D. Lorenz, Howard A. Zebker, Tom G. Farr, K. L. Mitchell, Richard West, E. L. Schaller, Giuseppe Mitri, Bryan Stiles, Lauren Wye
Publikováno v:
Icarus. 211:672-685
Titan’s enigmatic Xanadu province has been seen in some detail with instruments from the Cassini spacecraft. The region contains some of the most rugged, mountainous terrain on Titan, with relief over 2000 m. Xanadu contains evolved and integrated
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad276b9f40ca6714664f2fa6662efaad
https://doi.org/10.1016/j.icarus.2010.07.022
https://doi.org/10.1016/j.icarus.2010.07.022
Publikováno v:
Icarus. 208:385-394
Radarclinometry is a powerful technique for estimating heights of landforms in synthetic aperture radar (SAR) images of planetary surfaces. In particular, it has been used to estimate heights of dunes in the sand seas of Saturn’s moon Titan (Lorenz
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::770d13b23d0a03921faa1fe4a936f021
https://doi.org/10.1016/j.icarus.2010.01.023
https://doi.org/10.1016/j.icarus.2010.01.023
Autor:
Alberto Adriani, T. B. McCord, Robert H. Brown, Jason W. Barnes, Angioletta Coradini, Dale P. Cruikshank, Philip D. Nicholson, Federico Tosi, Roberto Seu, M. A. Janssen, Roberto Orosei, Jason M. Soderblom, A. I. Gavrishin, Jonathan I. Lunine, Fabrizio Capaccioni, Enrico Flamini, A. Negrão, Roger N. Clark, Richard D. West, Lauren Wye, Gianrico Filacchione, S. D. Wall, Maria Luisa Moriconi, Priscilla Cerroni
Publikováno v:
Icarus (N.Y.N.Y. 1962) 208 (2010): 366–384. doi:10.1016/j.icarus.2010.02.003
info:cnr-pdr/source/autori:Tosi F.,a; R. Orosei,a; R. Seu,b; A. Coradini,a; J.I. Lunine,a,c; G. Filacchione,d; A.I. Gavrishin,e; F. Capaccioni,d;P. Cerroni,d; A. Adriani,a; M.L. Moriconi,f; A. Negrão,g; E. Flamini,h; R.H. Brown,i; L.C. Wye,j; M. Janssen,k;R.D. West,k; J.W. Barnes,l; S.D. Wall,k; R.N. Clark,m; D.P. Cruikshank,n; T.B. McCord,o; P.D. Nicholson,p;J.M. Soderblom,i/titolo:Correlations between VIMS and RADAR data over the surface of Titan:Implications for Titan's surface properties/doi:10.1016%2Fj.icarus.2010.02.003/rivista:Icarus (N.Y.N.Y. 1962)/anno:2010/pagina_da:366/pagina_a:384/intervallo_pagine:366–384/volume:208
info:cnr-pdr/source/autori:Tosi F.,a; R. Orosei,a; R. Seu,b; A. Coradini,a; J.I. Lunine,a,c; G. Filacchione,d; A.I. Gavrishin,e; F. Capaccioni,d;P. Cerroni,d; A. Adriani,a; M.L. Moriconi,f; A. Negrão,g; E. Flamini,h; R.H. Brown,i; L.C. Wye,j; M. Janssen,k;R.D. West,k; J.W. Barnes,l; S.D. Wall,k; R.N. Clark,m; D.P. Cruikshank,n; T.B. McCord,o; P.D. Nicholson,p;J.M. Soderblom,i/titolo:Correlations between VIMS and RADAR data over the surface of Titan:Implications for Titan's surface properties/doi:10.1016%2Fj.icarus.2010.02.003/rivista:Icarus (N.Y.N.Y. 1962)/anno:2010/pagina_da:366/pagina_a:384/intervallo_pagine:366–384/volume:208
We apply a multivariate statistical method to Titan data acquired by different instruments onboard the Cassini spacecraft. We have searched through Cassini/VIMS hyperspectral cubes, selecting those data with convenient viewing geometry and that overl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd1ed7436ec4c2dd792ec037d71e034d
https://doi.org/10.1016/j.icarus.2010.02.003
https://doi.org/10.1016/j.icarus.2010.02.003
Autor:
Howard A. Zebker, Steven J. Ostro, Philip S. Callahan, Richard West, Bryan Stiles, Ralph D. Lorenz, C. Veeramachaneni, M. A. Janssen, G. Hamilton, K. Kelleher, William T. K. Johnson, Y. Anderson, Yonggyu Gim, Lauren Wye, R. Boehmer
Publikováno v:
Icarus. 206:498-506
Cassini radar tracks on Saturn’s icy satellites through the end of the Prime Mission in 2008 have increased the number of radar albedo estimates from 10 ( Ostro et al., 2006 ) to 73. The measurements sample diverse subradar locations (and for Dione
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2521b9cdc9033002533322351f74eeca
https://doi.org/10.1016/j.icarus.2009.07.041
https://doi.org/10.1016/j.icarus.2009.07.041
Autor:
M. A. Janssen, L. A. Soderblom, Flora Paganelli, A. Legall, Ralph D. Lorenz, Jani Radebaugh, Jonathan I. Lunine, Philip S. Callahan, Karl L. Mitchell, J. Craig, Bryan Stiles, S. D. Wall, R.J. Ollerenshaw, Ellen R. Stofan, R. Peckyno, Charles A. Wood, Alexander G. Hayes, Randolph L. Kirk, Robert West, P. Valora, Rosaly M. C. Lopes, Tom G. Farr, Y. Anderson, Giuseppe Mitri, Lauren Wye
Publikováno v:
Icarus. 205:540-558
The Cassini Titan Radar Mapper is providing an unprecedented view of Titan’s surface geology. Here we use Synthetic Aperture Radar (SAR) image swaths (Ta–T30) obtained from October 2004 to December 2007 to infer the geologic processes that have s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b5e80786a22e98bf365cb9d6a1a7a860
https://doi.org/10.1016/j.icarus.2009.08.010
https://doi.org/10.1016/j.icarus.2009.08.010