Publications
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Abstracts of the Annual Meeting of Planetary Geologic Mappers, Tucson, AZ 2007 Abstracts of the Annual Meeting of Planetary Geologic Mappers, Tucson, AZ 2007
Introduction Report of the Annual Mappers Meeting Planetary Science Institute Tucson, Arizona June 28 and 29, 2007 Approximately 22 people attended this year's mappers meeting, and many more submitted abstracts and maps in absentia. The 2007 meeting was convened by Tracy Gregg, Les Bleamaster, Steve Saunders, and Ken Tanaka and was hosted by David Crown and Les Bleamaster of the...
Authors
Tracy Gregg, Kenneth L. Tanaka, R. Stephen Saunders
Ultrahigh resolution topographic mapping of Mars with HiRISE stereo images: Methods and first results Ultrahigh resolution topographic mapping of Mars with HiRISE stereo images: Methods and first results
The Mars Reconnaissance Orbiter (MRO) arrived at Mars on 10 March 2006 and began its primary science phase in November. The High Resolution Imaging Science Experiment (HiRISE) on MRO is the largest, most complex camera ever flown to another planet. Plans call for this scanner to image roughly 1% of Mars by area at a pixel scale of 0.3 m during the next Mars year. Among the thousands of...
Authors
Randolph L. Kirk, Elpitha Howington-Kraus, Mark R. Rosiek, Debbie Cook, Jeffery A. Anderson, Kris J. Becker, Brent A. Archinal, Laszlo P. Keszthelyi, R. King, Alfred S. McEwen
Cartography for lunar exploration: Current status and planned missions Cartography for lunar exploration: Current status and planned missions
The initial spacecraft exploration of the Moon in the 1960s–70s yielded extensive data, primarily in the form of film and television images, that were used to produce a large number of hardcopy maps by conventional techniques. A second era of exploration, beginning in the early 1990s, has produced digital data including global multispectral imagery and altimetry, from which a new...
Authors
Randolph L. Kirk, Brent A. Archinal, Lisa R. Gaddis, Mark R. Rosiek
Mars Global Digital Dune Database: MC2-MC29 Mars Global Digital Dune Database: MC2-MC29
Introduction The Mars Global Digital Dune Database presents data and describes the methodology used in creating the database. The database provides a comprehensive and quantitative view of the geographic distribution of moderate- to large-size dune fields from 65? N to 65? S latitude and encompasses ~ 550 dune fields. The database will be expanded to cover the entire planet in later...
Authors
Rosalyn K. Hayward, Kevin F. Mullins, L.K. Fenton, T.M. Hare, T.N. Titus, M.C. Bourke, Anthony Colaprete, P. R. Christensen
Mars: Surface and Interior Mars: Surface and Interior
No abstract available.
Report on the final completion of the Unified Lunar Control Network 2005 and Lunar Topographic Model Report on the final completion of the Unified Lunar Control Network 2005 and Lunar Topographic Model
In order to highlight this project to the extraterrestrial mapping community, we repeat here our earlier abstract [1], with a corrected Figure 2. A report describing the Unified Lunar Control Network 2005 and the files associated with that network is now available as an on-line USGS Open-File Report [2] at the location http://pubs.usgs.gov/of/2006/1367/. A “Readme” file describes the...
Authors
Brent A. Archinal, Mark R. Rosiek, Randolph L. Kirk, Trent M. Hare, Bonnie L. Redding
First stereoscopic radar images of Titan First stereoscopic radar images of Titan
Saturn's giant, cloud-covered satellite Titan, larger than the planet Mercury, is the last major piece of unexplored real estate in the Solar system. The NASA/ESA Cassini spacecraft carries a variety of instruments that are being used to map the surface of Titan, including optical instruments that provide a global synoptic view and spectroscopic information, and microwave imager (Cassini...
Authors
Randolph L. Kirk, Elpitha Howington-Kraus, K. L. Mitchell, S. Hensley, B.W. Stiles
Urgent processing and control of lunar data Urgent processing and control of lunar data
There is an urgent, time-critical need to begin tying together (geodetically controlling) all past and current lunar data, and to establish the cartographic foundation needed to make maximum use of future planned lunar data. Proper control of lunar datails required to properly support both lunar science and exploration, and at present we know of no plans within NASA to fund such work...
Authors
Brent A. Archinal, Lisa R. Gaddis, Randolph L. Kirk, Trent M. Hare, Mark R. Rosiek
Resolution effects in radarclinometry Resolution effects in radarclinometry
Data from the Cassini-Huygens mission, in particular images from the Cassini Titan Radar Mapper (RADAR) have revealed Saturn's giant moon, Titan to be a world whose geologic diversity and complexity approach those of the Earth itself. Estimates of topographic relief are, naturally, of enormous interest in the effort to understand the nature of Titan's surface features and quantify the...
Authors
Randolph L. Kirk, Jani Radebaugh
The HRSC DTM test The HRSC DTM test
The High Resolution Stereo Camera (HRSC, [1]) is part of the orbiter payload on the Mars Express (MEX) mission of the European Space Agency (ESA), orbiting the Red Planet in a highly elliptical orbit since January 2004. For the first time in planetary exploration, a camera system has especially been designed to meet the requirements of photogrammetry and cartography for mapping the...
Authors
Christian Heipke, Jurgen Oberst, Jeorg Albertz, Maria Attwenger, Peter Dorninger, Egon Dorrer, M. Ewe, Stephan Gehrke, Klaus Gwinner, H. Hirschmuller, J.R. Kim, Randolph L. Kirk, H. Mayer, Jan-Peter Muller, Rajagopalan Rengarajan, M. Rentsch, R. Schmidt, Frank Scholten, J. Shan, Michael Spiegel, M. Wahlisch, Gerhard Neukum
Vertical distribution of hydrogen at high northern latitudes on Mars: The Mars Odyssey Neutron Spectrometer Vertical distribution of hydrogen at high northern latitudes on Mars: The Mars Odyssey Neutron Spectrometer
Neutron leakage currents measured using the Mars Odyssey Neutron Spectrometer are used to develop a two‐layer model of the distribution of hydrogen (here parameterized as water‐equivalent hydrogen, WEH) at high northern latitudes. The WEH abundance in the upper layer, Wup, was found to range between 1% and about 5%. The maximum value of the apparent thickness, D, of this upper layer...
Authors
William C. Feldman, Michael T. Mellon, Olivier Gasnault, B. Diez, R.C. Elphic, Justin Hagerty, D. J. Lawrence, S. Maurice, T.H. Prettyman
Landsat ETM+ False-Color Image Mosaics of Afghanistan Landsat ETM+ False-Color Image Mosaics of Afghanistan
In 2005, the U.S. Agency for International Development and the U.S. Trade and Development Agency contracted with the U.S. Geological Survey to perform assessments of the natural resources within Afghanistan. The assessments concentrate on the resources that are related to the economic development of that country. Therefore, assessments were initiated in oil and gas, coal, mineral...
Authors
Philip A. Davis