Zobrazeno 1 - 10
of 104
pro vyhledávání: '"Laurence A. Soderblom"'
Autor:
Paul E. Geissler, Timothy N. Titus, Laurence A. Soderblom, William M. Grundy, David P. Mayer, Jeffrey R. Johnson, Justin J. Hagerty, R. Greg Vaughan
Publikováno v:
Advanced Applications in Remote Sensing of Agricultural Crops and Natural Vegetation ISBN: 9780429431166
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ab57841dd445303291f4669d457e2790
https://doi.org/10.1201/9780429431166-14
https://doi.org/10.1201/9780429431166-14
Autor:
Shannon MacKenzie, Alexander G. Hayes, Laurence A. Soderblom, Jason W. Barnes, Eliot F. Young, Christophe Sotin, Jason M. Soderblom, Robert H. Brown
Publikováno v:
The Planetary Science Journal. 1:24
The selection of Dragonfly enables regional Titan surface science, but global Titan geophysics, geology, hydrology, and meteorology require an orbiter. We consider the sources of signal and noise that would contribute to near-infrared surface imaging
Autor:
Jonathan I. Lunine, Michael Janssen, Rosaly M. C. Lopes, Philip D. Nicholson, Ellen R. Stofan, Laurence A. Soderblom, Jason W. Barnes, Kevin H. Baines, Ralf Jaumann, Bonnie J. Buratti, Roger N. Clark, Ralph D. Lorenz, Thomas B. McCord, Dale P. Cruikshank, Charles Elachi, Jeffrey A. Anderson, T. Sucharski, Erich Karkoschka, Christophe Sotin, Randolph L. Kirk, Martin G. Tomasko, Jani Radebaugh, Stephen D. Wall, Stéphane Le Mouélic, Robert H. Brown, Janet M. Barrett, Bashar Rizk
Publikováno v:
Planetary and Space Science. 55:2025-2036
Titan's vast equatorial fields of RADAR-dark longitudinal dunes seen in Cassini RADAR synthetic aperture images correlate with one of two dark surface units discriminated as “brown” and “blue” in Visible and Infrared Mapping Spectrometer (VIM
Autor:
Robert H. Brown, Roger V. Yelle, David Thomas, Patricia Beauchamp, Meemong Lee, David H. Rodgers, Robert T. Benoit, Gun Shing Chen, Laurence A. Soderblom, Bill R. Sandel
Publikováno v:
Space Science Reviews. 129:309-326
MICAS is an integrated multi-channel instrument that includes an ultraviolet imaging spectrometer (80–185 nm), two high-resolution visible imagers (10–20 μrad/pixel, 400–900 nm), and a short-wavelength infrared imaging spectrometer (1250–260
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:
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
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:
William H. Farrand, James F. Bell, B. C. Hahn, Scott M. McLennan, Steven W. Squyres, Jeffrey R. Johnson, Philip R. Christensen, Sarah Stewart Johnson, Harry Y. McSween, David A. Fike, J. M. Pocock, A. Ghosh, Nicholas J. Tosca, Michael C. Malin, Michael B. Wyatt, Kenneth E. Herkenhoff, Jack D. Farmer, Joel A. Hurowitz, Wendy M. Calvin, P. A. de Souza, Wesley A. Watters, Timothy D. Glotch, Bradley L. Jolliff, Z. A. Learner, Ralf Gellert, John P. Grotzinger, Benton C. Clark, Laurence A. Soderblom, Albert S. Yen, Steven W. Ruff, Andrew H. Knoll, Göstar Klingelhöfer
Publikováno v:
Earth and Planetary Science Letters. 240:95-121
Impure reworked evaporitic sandstones, preserved on Meridiani Planum, Mars, are mixtures of roughly equal amounts of altered siliciclastic debris, of basaltic provenance (40 ± 10% by mass), and chemical constituents, dominated by evaporitic minerals
Publikováno v:
Photogrammetric Engineering & Remote Sensing. 71:1167-1178
Analysis of data combining daytime visible reflected, daytime IR emitted, and nighttime IR emitted images allows us to isolate the physical effects of topography, albedo, and thermal inertia. To a good approximation, these physical influences interac
Autor:
Harry Y. McSween, J. Brückner, Wendy M. Calvin, William M. Folkner, Scott M. McLennan, J. W. Rice, G. Landis, Matthew P. Golombek, Philip R. Christensen, R. Li, David J. Des Marais, Jeffrey E. Moersch, Steven W. Squyres, Paul S. Smith, John A. Grant, Göstar Klingelhöfer, James F. Bell, Jeffrey R. Johnson, Thanasis E. Economou, Kenneth E. Herkenhoff, Heinrich Wänke, Michael C. Malin, Jack D. Farmer, Laurence A. Soderblom, N. A. Cabrol, Benton C. Clark, John P. Grotzinger, Morten Madsen, Ronald Greeley, Michael H. Carr, Claude d’Uston, T. J. Parker, M. Sims, S. P. Gorevan, M. J. Wolff, Thomas J. Wdowiak, Stubbe F. Hviid, M. D. Smith, Andrew H. Knoll, Albert S. Yen, Mark T. Lemmon, Rudolf Rieder, Larry S. Crumpler, William H. Farrand, Larry A. Haskin, D. W. Ming, Ryan C. Sullivan, Raymond E. Arvidson, Richard V. Morris, Lutz Richter
Publikováno v:
Science. 306:1698-1703
The Mars Exploration Rover Opportunity has investigated the landing site in Eagle crater and the nearby plains within Meridiani Planum. The soils consist of fine-grained basaltic sand and a surface lag of hematite-rich spherules, spherule fragments,