Megaflood analysis through channel networks of the Athabasca Valles, Mars based on multi-resolution stereo DTMs and 2D hydrodynamic modeling
暂无分享,去创建一个
[1] Jeffrey B. Plescia,et al. Cerberus Fossae, Elysium, Mars: a source for lava and water , 2003 .
[2] Paul D. Bates,et al. Improving the stability of a simple formulation of the shallow water equations for 2‐D flood modeling , 2012 .
[3] W. Hartmann,et al. Elysium Planitia lava flows: Crater count chronology and geological implications , 2000 .
[4] J. Murray,et al. Stratigraphical and morphological evidence for pingo genesis in the Cerberus plains , 2006 .
[5] M. Manga. Martian floods at Cerberus Fossae can be produced by groundwater discharge , 2004 .
[6] N. Hoffman. White Mars: A New Model for Mars' Surface and Atmosphere Based on CO2 , 2000 .
[7] David E. Smith,et al. Mars Orbiter Laser Altimeter: Experiment summary after the first year of global mapping of Mars , 2001 .
[8] Yun-Soo Choi,et al. Toward generalized planetary stereo analysis scheme—Prototype implementation with multi-resolution Martian stereo imagery , 2013, Earth, Planets and Space.
[9] A. McEwen,et al. Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE) , 2007 .
[10] Randolph L. Kirk,et al. The rayed crater Zunil and interpretations of small impact craters on Mars , 2005 .
[11] P. Bates,et al. A simple inertial formulation of the shallow water equations for efficient two-dimensional flood inundation modelling. , 2010 .
[12] J. Emery,et al. Young (late Amazonian), near-surface, ground ice features near the equator, Athabasca Valles, Mars , 2005 .
[13] T. Parker,et al. Extraterrestrial coastal geomorphology , 2001 .
[14] Jan-Peter Muller,et al. An assessment of surface matching for the automated co-registration of MOLA, HRSC and HiRISE DTMs , 2010 .
[15] J. Muller,et al. Hydraulic modeling of a distributary channel of Athabasca Valles, Mars, using a high-resolution digital terrain model , 2012 .
[16] B. Lucchitta. Ice sculpture in the Martian outflow channels , 1982 .
[17] S. Kanae,et al. A physically based description of floodplain inundation dynamics in a global river routing model , 2011 .
[18] A. McEwen,et al. Ultrahigh resolution topographic mapping of Mars with MRO HiRISE stereo images: Meter‐scale slopes of candidate Phoenix landing sites , 2008 .
[19] Jeong-Woo Hong,et al. Implementation of Martian virtual reality environment using very high-resolution stereo topographic data , 2012, Comput. Geosci..
[20] L. Edwards,et al. Context Camera Investigation on board the Mars Reconnaissance Orbiter , 2007 .
[21] A. McEwen,et al. Repeated Aqueous Flooding from the Cerberus Fossae: Evidence for Very Recently Extant, Deep Groundwater on Mars , 2002 .
[22] J. Muller,et al. The Western Elysium Planitia Paleolake , 2010 .
[23] Paul D. Bates,et al. How much physical complexity is needed to model flood inundation? , 2012 .
[24] L. Keszthelyi,et al. Initial insights from 2.5D hydraulic modeling of floods in Athabasca Valles, Mars , 2007 .
[25] Kenneth L. Tanaka. Debris‐flow origin for the Simud/Tiu deposit on Mars , 1999 .
[26] P. Grindrod,et al. Topographic, spectral and thermal inertia analysis of interior layered deposits in Iani Chaos, Mars , 2012 .
[27] J. Muller,et al. Multi-resolution topographic data extraction from Martian stereo imagery , 2009 .
[28] L. Wilson,et al. Megaflooding on Earth and Mars: Dynamics of fluid flow in Martian outflow channels , 2009 .
[29] D. Burr. Hydraulic modelling of Athabasca Vallis, Mars , 2003 .
[30] Christian Heipke,et al. Topography of Mars from global mapping by HRSC high-resolution digital terrain models and orthoimages: Characteristics and performance , 2010 .
[31] Jan-Peter Muller,et al. Evidence from the Mars Express High Resolution Stereo Camera for a frozen sea close to Mars' equator , 2005, Nature.
[32] F. Poulet,et al. Ismenius Cavus, Mars: A deep paleolake with phyllosilicate deposits , 2010 .
[33] A. McEwen,et al. Recent aqueous floods from the Cerberus Fossae, Mars , 2002 .
[34] W. Luo,et al. Morphometric analysis of Martian valley network basins using a circularity function , 2005 .
[35] Takeo Kanade,et al. A Cooperative Algorithm for Stereo Matching and Occlusion Detection , 2000, IEEE Trans. Pattern Anal. Mach. Intell..
[36] F. Scholten,et al. Mars Express HRSC Data Processing - Methods and Operational Aspects , 2005 .
[37] T. Stepinski,et al. Morphology of drainage basins as an indicator of climate on early Mars , 2005 .
[38] David E. Smith,et al. Crossover analysis of Mars Orbiter Laser Altimeter data , 2001 .
[39] Lionel Wilson,et al. Generation of recent massive water floods at Cerberus Fossae, Mars by dike emplacement, cryospheric cracking, and confined aquifer groundwater release , 2003 .
[40] J. Muller,et al. Evaluating planetary digital terrain models - the HRSC DTM test , 2007 .
[41] Randolph L. Kirk,et al. Fluvial channels on Titan: Initial Cassini RADAR observations , 2008 .
[42] Jan-Peter Muller,et al. A refined chronology of catastrophic outflow events in Ares Vallis, Mars , 2009 .
[43] Mark R. Rosiek,et al. Emplacement of the youngest flood lava on Mars: A short, turbulent story , 2010 .
[44] P. Bates,et al. A subgrid channel model for simulating river hydraulics and floodplain inundation over large and data sparse areas , 2012 .
[45] A. Gruen. ADAPTIVE LEAST SQUARES CORRELATION: A POWERFUL IMAGE MATCHING TECHNIQUE , 1985 .
[46] Alfred S. McEwen,et al. Athabasca Valles, Mars: A Lava-Draped Channel System , 2007, Science.
[47] J. Muller,et al. Multi-resolution digital terrain models and their potential for Mars landing site assessments , 2013 .