- DSpace Home
- →
- Browsing by Author
JavaScript is disabled for your browser. Some features of this site may not work without it.
Browsing by Author "Irwin, Rossman P., III"
Now showing items 1-20 of 36
-
Grant, John A.; Irwin, Rossman P., III; Wilson, Sharon A. (Elsevier, 2010)
-
Constraints on the Noachian paleoclimate of the martian highlands from landscape evolution modeling Matsubara, Yo; Howard, Alan D.; Irwin, Rossman P., III (2018)The progressive degradation and loss of impact craters throughout the Noachian Period on Mars indicate prolonged erosion, rather than a brief spike around the Noachian/Hesperian transition. The purpose of this study is to ...
-
Irwin, Rossman P., III; Cawley, Jon C. (Smithsonian National Air and Space Museum - Center for Earth and Planetary Studies, 2019)This data repository contains Mars Odyssey Thermal Emission Imaging System base mosaics (592.75 pixels/degree), Mars Global Surveyor Mars Orbiter Laser Altimeter gridded topography (128 pixels/degree), and ArcGIS polygon ...
-
Matsubara, Yo; Howard, Alan D.; Irwin, Rossman P., III (Smithsonian National Air and Space Museum - Center for Earth and Planetary Studies, 2018)This data repository includes the Fortran source files for landscape evolution modeling, initial conditions digital elevation models (DEMs), example model result DEMs, image mosaics, and topographic DEMs for two study areas ...
-
Irwin, Rossman P., III; Tanaka, Kenneth L.; Robbins, Stuart J. (2013)Most of the geomorphic changes on Mars occurred during the Noachian Period, when the rates of impact crater degradation and valley network incision were highest. Fluvial erosion around the Noachian/Hesperian transition is ...
-
Irwin, Rossman P., III; Howard, A. D. (2002)None
-
Craddock, Robert A.; Howard, Alan D.; Irwin, Rossman P., III; Tooth, Stephen; Williams, Rebecca M. E.; Chu, Pao-Shin (2012)
-
Williams, R. M. E.; Irwin, Rossman P., III; Zimbelman, James R. (2009)
-
Cawley, Jon C.; Irwin, Rossman P., III (2018)Extensive Noachian-aged intercrater planation surfaces comprise much of the southern highlands of Mars. We mapped aggradational and stable to degradational surfaces in three study areas with diverse relief elements and ...
-
Williams, Rebecca M. E.; Irwin, Rossman P., III; Zimbelman, James R.; Chidsey, Thomas C., Jr.; Eby, David E. (Geological Society of America, 2011)
-
Burr, Devon M.; Perron, J. T.; Lamb, Michael P.; Irwin, Rossman P., III; Collins, Geoffrey C.; Howard, Alan D.; Sklar, Leonard S.; Moore, Jeffrey M.; Adamkovics, Mate; Baker, Victor R.; Drummond, Sarah, A.; Black, Benjamin A. (2013)
-
Irwin, Rossman P., III; Howard, A. D.; Craddock, Robert A. (John Wiley & Sons Ltd, 2008)
-
Weitz, Catherine M.; Irwin, Rossman P., III; Chuang, F. C.; Bourke, M. C.; Crown, D. A. (2006)
-
Tanaka, Kenneth L.; Skinner Jr, James A.; Dohm, James M.; Irwin, Rossman P., III; Kolb, Eric J.; Fortezzo, Corey M.; Platz, Thomas; Michael, Gregory G.; Hare, Trent M. (USGS, 2014)
-
Irwin, Rossman P., III; Grant, John A. (USGS, 2013)
-
Irwin, Rossman P., III; Mest, Scott C. (Smithsonian National Air and Space Museum - Center for Earth and Planetary Studies, 2018)This data repository includes a 1:1,000,000 scale ArcGIS 10.5 map of geologic units, craters, other structures, and valleys in a study area in Terra Sabaea, Mars, bounded by 19–22°S, 40.4–45.4°E. Base image mosaics are ...
-
Irwin, Rossman P., III; Watters, Thomas R. (2010)The contrast in crustal thickness, surface age, elevation, and morphology between the southern cratered highlands and northern lowland plains of Mars is termed the crustal dichotomy. The oldest exposed sections of the ...
-
Irwin, Rossman P., III; Howard, A. D.; Maxwell, Ted A. (2004)None
-
Watters, Thomas R.; McGovern, P. J.; Irwin, Rossman P., III (2007)None
-
Grant, John A.; Irwin, Rossman P., III; Grotzinger, John P.; Milliken, Ralph E.; Tornabene, Livio L.; McEwen, Alfred S.; Weitz, Catherine M.; Squyres, Steven W.; Glotch, Timothy D.; Thomson, Brad J. (2008)
Now showing items 1-20 of 36
Search DSpace
Browse
-
All of DSpace
