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Research Article| October 01, 1988 Flood surfaces and deflation surfaces within the Cutler Formation and Cedar Mesa Sandstone (Permian), southeastern Utah RICHARD LANGFORD; RICHARD LANGFORD 1Department of Geology and Geophysics, University of Utah, Salt Lake City, Utah 84112 Search for other works by this author on: GSW Google Scholar MARJORIE A. CHAN MARJORIE A. CHAN 1Department of Geology and Geophysics, University of Utah, Salt Lake City, Utah 84112 Search for other works by this author on: GSW Google Scholar Author and Article Information RICHARD LANGFORD 1Department of Geology and Geophysics, University of Utah, Salt Lake City, Utah 84112 MARJORIE A. CHAN 1Department of Geology and Geophysics, University of Utah, Salt Lake City, Utah 84112 Publisher: Geological Society of America First Online: 01 Jun 2017 Online ISSN: 1943-2674 Print ISSN: 0016-7606 Geological Society of America GSA Bulletin (1988) 100 (10): 1541–1549. https://doi.org/10.1130/0016-7606(1988)100<1541:FSADSW>2.3.CO;2 Article history First Online: 01 Jun 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn Email Permissions Search Site Citation RICHARD LANGFORD, MARJORIE A. CHAN; Flood surfaces and deflation surfaces within the Cutler Formation and Cedar Mesa Sandstone (Permian), southeastern Utah. GSA Bulletin 1988;; 100 (10): 1541–1549. doi: https://doi.org/10.1130/0016-7606(1988)100<1541:FSADSW>2.3.CO;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 SocietyGSA Bulletin Search Advanced Search Abstract Areally extensive erosion surfaces in eolian deposits have been interpreted as long hiatuses in eolian deposition. Such erosion surfaces form during deflationary episodes or during periods of erg stabilization or contraction. They are called "super surfaces" and can be useful for stratigraphic correlation because of their regional extent.The Permian Cedar Mesa Sandstone and Cutler Formation contain a type off super surface (herein termed "flood surfaces"), ∼10-400+ km2. Flood surfaces form as a result of fluvial floods into active dune seas. The surfaces may expand through nonclimbing migration of eolian dunes but do not imply long hiatuses in eolian deposition as do other types of super surfaces. Cutler and Cedar Mesa flood surfaces are overlain by shales and sandstones which thicken laterally and merge with fluvial channel-fill deposits. Flooding of active dune fields in the Cedar Mesa Sandstone is suggested by intertonguing of eolian dune and fluvial deposits. Flood surfaces can easily be mistaken for deflationary super surfaces but are distinguished by evidence of dune migration coincident with flood events and by an increase in the number of surfaces adjacent to associated aqueous deposits. This content is PDF only. Please click on the PDF icon to access. First Page Preview Close Modal 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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Langford et al. (1988) studied this question.
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