Abstract

Research Article| April 01, 2004 Hydrogeologic processes of large-scale tectonomagmatic complexes in Mongolia–southern Siberia and on Mars Goro Komatsu; Goro Komatsu 1International Research School of Planetary Sciences, Università d'Annunzio, Viale Pindaro 42, 65127 Pescara, Italy Search for other works by this author on: GSW Google Scholar James M. Dohm; James M. Dohm 2Department of Hydrology and Water Resources, University of Arizona, Tucson, Arizona 85721, USA Search for other works by this author on: GSW Google Scholar Trent M. Hare Trent M. Hare 3U.S. Geological Survey, Flagstaff, Arizona 86001, USA Search for other works by this author on: GSW Google Scholar Author and Article Information Goro Komatsu 1International Research School of Planetary Sciences, Università d'Annunzio, Viale Pindaro 42, 65127 Pescara, Italy James M. Dohm 2Department of Hydrology and Water Resources, University of Arizona, Tucson, Arizona 85721, USA Trent M. Hare 3U.S. Geological Survey, Flagstaff, Arizona 86001, USA Publisher: Geological Society of America Received: 25 Sep 2003 Revision Received: 30 Dec 2003 Accepted: 31 Dec 2003 First Online: 02 Mar 2017 Online ISSN: 1943-2682 Print ISSN: 0091-7613 Geological Society of America Geology (2004) 32 (4): 325–328. https://doi.org/10.1130/G20237.2 Article history Received: 25 Sep 2003 Revision Received: 30 Dec 2003 Accepted: 31 Dec 2003 First Online: 02 Mar 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation Goro Komatsu, James M. Dohm, Trent M. Hare; Hydrogeologic processes of large-scale tectonomagmatic complexes in Mongolia–southern Siberia and on Mars. Geology 2004;; 32 (4): 325–328. doi: https://doi.org/10.1130/G20237.2 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyGeology Search Advanced Search Abstract Large-scale tectonomagmatic complexes are common on Earth and Mars. Many of these complexes are created or at least influenced by mantle processes, including a wide array of plume types ranging from superplumes to mantle plumes. Among the most prominent complexes, the Mongolian plateau on Earth and the Tharsis bulge on Mars share remarkable similarities in terms of large domal uplifted areas, great rift canyon systems, and widespread volcanism on their surfaces. Water has also played an important role in the development of the two complexes. In general, atmospheric and surface water play a bigger role in the development of the present-day Mongolian plateau than for the Tharsis bulge, as evidenced by highly developed drainages and thick accumulation of sediments in the basins of the Baikal rift system. On the Tharsis bulge, however, water appears to have remained as ground ice except during periods of elevated magmatic activity. Glacial and periglacial processes are well documented for the Mongolian plateau and are also reported for parts of the Tharsis bulge. Ice-magma interactions, which are represented by the formation of subice volcanoes in parts of the Mongolian plateau region, have been reported for the Valles Marineris region of Mars. The complexes are also characterized by cataclysmic floods, but their triggering mechanism may differ: mainly ice-dam failures for the Mongolian plateau and outburst of groundwater for the Tharsis bulge, probably by magma-ice interactions, although ice-dam failures within the Valles Marineris region cannot be ruled out as a possible contributor. Comparative studies of the Mongolian plateau and Tharsis bulge provide excellent opportunities for understanding surface manifestations of plume-driven processes on terrestrial planets and how they interact with hydro-cryospheres. You do not have access to this content, please speak to your institutional administrator if you feel you should have access.

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