Publications
Filter Total Items: 915
Utility of Viking Orbiter images and products for Mars mapping
This paper reports on mapping procedures developed by the U.S. Geological Survey that use Viking Orbiter imagery and Mars Orbiter Laser Altimeter (MOLA) derived radii to produce topographic data. The use of Mosaiced Digital Image Models (MDIMs), created from Viking Orbiter images, and MOLA data to provide horizontal and vertical control is reviewed. We describe procedures to adapt a commercial dig
Authors
Mark R. Rosiek, Randolph L. Kirk, Brent A. Archinal, Elpitha Howington-Kraus, Trent M. Hare, Donna M. Galuszka, Bonnie L. Redding
Three in one: Multiscale Hardcopy Depiction of the Mars Surface in True3D
The visualisation of both geospatial Earth data and extra-terrestrial objects is gain- ing increasing importance. Until recently, hardcopy displays were confined to mostly static, two-dimensional or pseudo-three-dimensional depictions. The various effects offered by lenticular foil technology allow the generation of flip-image effects, short animations, and true-3D displays in hardcopy form. One a
Authors
Manfred Buchroithner, Thomas Gründemann, Randolph L. Kirk, Klaus Habermann
Initial results of rover localization and topographic mapping for the 2003 mars exploration rover mission
This paper presents the initial results of lander and rover localization and topographic mapping of the MER 2003 mission (by Sol 225 for Spirit and Sol 206 for Opportunity). The Spirit rover has traversed a distance of 3.2 km (actual distance traveled instead of odometry) and Opportunity at 1.2 km. We localized the landers in the Gusev Crater and on the Meridiani Planum using two-way Doppler radio
Authors
Rongxing Li, Steven W. Squyres, Raymond E. Arvidson, Brent A. Archinal, James F. Bell, Yang Cheng, Larry S. Crumpler, David J. Des Marais, Kaichang Di, Todd A. Ely, Matthew P. Golombek, Eric Graat, John Grant, Joe Guinn, Andrew C. Johnson, Ronald Greeley, Randolph L. Kirk, Mark Maimone, Laurence A. Soderblom, Shane D. Thompson, Jue Wang, Patrick L. Whelley, Fengliang Xu
Joint analysis of visible and infrared images
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 interact linearly so that maps showing topographic shading, albedo, and relative thermal inertia can be produced by simple algebraic manipulation of the co-r
Authors
Randolph L. Kirk, Laurence A. Soderblom, Glen E. Cushing, Timothy A. Tituus
HRSC on Mars Express: Photogrammetric and cartographic research
The High Resolution Stereo Camera (HRSC) on the European spacecraft Mars Express is the first camera on a planetary mission especially designed for photogrammetric and cartographic purposes. Since January 2004 the camera has been taking image data from the Martian surface, characterized by high-resolution, stereo capability and color. These data provide an enormous potential for the generation of
Authors
Jeorg Albertz, Maria Attwenger, Janet M. Barrett, Simon Casley, Peter Dorninger, Egon Dorrer, Heinrich Ebner, Stephan Gehrke, Bernd Giese, Klaus Gwinner, Christian Heipke, Elpitha Howington-Kraus, Randolph L. Kirk, Hartmut Lehmann, Helmut Mayer, Jan-Peter Muller, Juergen Oberst, Alexey Ostrovskiy, Joerg Renter, Sergiy Reznik, Ralph George Schmidt, Frank Scholten, Michael Spiegel, Uwe Stilla, Marita Wählisch, Gerhard Neukum
The rayed crater Zunil and interpretations of small impact craters on Mars
A 10-km diameter crater named Zunil in the Cerberus Plains of Mars created ∼107 secondary craters 10 to 200 m in diameter. Many of these secondary craters are concentrated in radial streaks that extend up to 1600 km from the primary crater, identical to lunar rays. Most of the larger Zunil secondaries are distinctive in both visible and thermal infrared imaging. MOC images of the secondary craters
Authors
Alfred S. McEwen, Brandon S. Preblich, Elizabeth P. Turtle, Natalia A. Artemieva, Matthew P. Golombek, Michelle Hurst, Randolph L. Kirk, Devon M. Burr, Phillip R. Christensen
Cassini radar views the surface of Titan
The Cassini Titan Radar Mapper imaged about 1% of Titan's surface at a resolution of ∼0.5 kilometer, and larger areas of the globe in lower resolution modes. The images reveal a complex surface, with areas of low relief and a variety of geologic features suggestive of dome-like volcanic constructs, flows, and sinuous channels. The surface appears to be young, with few impact craters. Scattering an
Authors
C. Elachi, S. Wall, M. Allison, Y. Anderson, R. Boehmer, P. Callahan, P. Encrenaz, E. Flamini, G. Franceschetti, Y. Gim, G. Hamilton, S. Hensley, M. Janssen, W. Johnson, K. Kelleher, Randolph L. Kirk, R. Lopes, R. Lorenz, J. Lunine, D. Muhleman, S. Ostro, F. Paganelli, G. Picardi, F. Posa, L. Roth, R. Seu, S. Shaffer, Laurence A. Soderblom, B. Stiles, E. Stofan, S. Vetrella, R. West, C. Wood, L. Wye, H. Zebker
Are there active glaciers on Mars? (Reply)
Gillespie et al.1 concur with our interpretation that certain lobate equatorial and mid-latitude features on Mars are due to debris-covered glaciers formed largely during past periods of increased spin-axis obliquity, when climate regimes favoured snow and ice accumulation and glacial flow2. They suggest that the ‘hourglass’ deposit, dated at more than 40 Myr old2, could be active today owing to a
Authors
J.W. Head, G. Neukum, R. Jaumann, H. Hiesinger, E. Hauber, M. H. Carr, P. Masson, B. Foing, H. Hoffmann, M. Kreslavsky, S. Milkovich, S. Van Gasselt
New Perspectives on Ancient Mars
Mars was most active during its first billion years. The core, mantle, and crust formed within ∼50 million years of solar system formation. A magnetic dynamo in a convecting fluid core magnetized the crust, and the global field shielded a more massive early atmosphere against solar wind stripping. The Tharsis province became a focus for volcanism, deformation, and outgassing of water and carbon di
Authors
S.C. Solomon, O. Aharonson, J.M. Aurnou, W. B. Banerdt, Michael H. Carr, A.J. Dombard, H. V. Frey, Matthew P. Golombek, S.A. Hauck, J.W. Head, Bruce M. Jakosky, C.L. Johnson, P.J. McGovern, G.A. Neumann, R.J. Phillips, D.E. Smith, Maria Zuber
Photogrammetric analysis of the Mars Global Surveyor mapping data
This paper studies the photogrammetric mapping properties and capabilities of the Mars Global Surveyor (MGS) mapping data. Starting from the raw MGS data, we decompress the MOC narrow angle images, extract, and calculate their exterior orientation from the SPICE kernels, and calculate the 3D coordinates of MOLA footprints from MOLA PEDR files. A new approach is proposed that registers a MOLA profi
Authors
Jie Shan, Jong-suk Yoon, D. Scott Lee, Randolph L. Kirk, Gregory Neumann, Charles H. Acton
An integrated view of the chemistry and mineralogy of martian soils
The mineralogical and elemental compositions of the martian soil are indicators of chemical and physical weathering processes. Using data from the Mars Exploration Rovers, we show that bright dust deposits on opposite sides of the planet are part of a global unit and not dominated by the composition of local rocks. Dark soil deposits at both sites have similar basaltic mineralogies, and could refl
Authors
A. S. Yen, Ralf Gellert, C. Schroder, R.V. Morris, J.F. Bell, A.T. Knudson, B. C. Clark, D. W. Ming, J.A. Crisp, R. E. Arvidson, D. Blaney, J. Brückner, P. R. Christensen, D.J. DesMarais, P.A. De Souza, T.E. Economou, A. Ghosh, B.C. Hahn, Kenneth E. Herkenhoff, L.A. Haskin, J.A. Hurowitz, B.L. Joliff, J. R. Johnson, G. Klingelhofer, M.B. Madsen, S. M. McLennan, H.Y. McSween, L. Richter, R. Rieder, D. Rodionov, Laurence A. Soderblom, S. W. Squyres, N.J. Tosca, A. Wang, M. Wyatt, J. Zipfel