2023 CSDMS meeting-103: Difference between revisions

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{{CSDMS meeting personal information template-2023
{{CSDMS meeting personal information template-2023
|CSDMS meeting first name=Sean
|CSDMS meeting first name=Joe
|CSDMS meeting last name=Gallen
|CSDMS meeting last name=Hughes
|CSDMS Pronouns=he/him
|CSDMS Pronouns=he/him
|CSDMS meeting institute=Department of Geosciences, Colorado State University
|CSDMS meeting institute=USGS
|CSDMS meeting city=Fort Collins
|CSDMS meeting city=Chicago
|CSDMS meeting country=United States
|CSDMS meeting country=United States
|CSDMS meeting state=CO
|CSDMS meeting state=CO
|CSDMS meeting email address=sean.gallen@colostate.edu
|CSDMS meeting email address=jdhughes@usgs.gov
|CSDMS meeting phone=3157297939
}}
}}
{{CSDMS meeting select clinics1 2023
{{CSDMS meeting select clinics1 2023
|CSDMS_meeting_select_clinics1_2023=3) Using GPUs to Solve Science Problems Faster
|CSDMS_meeting_select_clinics1_2023=5) Will not attend a clinic this day
}}
}}
{{CSDMS meeting select clinics2 2023
{{CSDMS meeting select clinics2 2023
|CSDMS_meeting_select_clinics2_2023=2) Coupling models of lithospheric deformation and surface processes (ASPECT)
|CSDMS_meeting_select_clinics2_2023=5) Will not attend a clinic this day
}}
}}
{{CSDMS meeting select clinics3 2023
{{CSDMS meeting select clinics3 2023
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{{CSDMS meeting abstract yes no 2023
{{CSDMS meeting abstract yes no 2023
|CSDMS meeting abstract submit 2023=Yes
|CSDMS meeting abstract submit 2023=No
}}
{{CSDMS meeting abstract poster Epub 2023
|CSDMS meeting poster Epub submit 2023=Poster
}}
{{CSDMS meeting abstract title temp2023
|CSDMS meeting abstract title=Slab-mantle interactions pace forearc uplift during subduction retreat in the Central Mediterranean
|Working_group_member_WG_FRG=Terrestrial Working Group, Geodynamics Focus Research Group
}}
{{CSDMS meeting authors template
|CSDMS meeting coauthor first name abstract=Nikki
|CSDMS meeting coauthor last name abstract=Seymour
|CSDMS meeting coauthor institute / Organization=Department of Geological Sciences, Stanford University
|CSDMS meeting coauthor town-city=Stanford
|CSDMS meeting coauthor country=United States
|State=California
}}
{{CSDMS meeting authors template
|CSDMS meeting coauthor first name abstract=Christoph
|CSDMS meeting coauthor last name abstract=Glotzbach
|CSDMS meeting coauthor institute / Organization=Department of Geosciences, University of Tübingen
|CSDMS meeting coauthor town-city=Tübingen
|CSDMS meeting coauthor country=Germany
}}
{{CSDMS meeting authors template
|CSDMS meeting coauthor first name abstract=Daniel
|CSDMS meeting coauthor last name abstract=Stockli
|CSDMS meeting coauthor institute / Organization=Department of Geological Sciences, University of Texas at Austin
|CSDMS meeting coauthor town-city=Austin
|CSDMS meeting coauthor country=United States
|State=Texas
}}
{{CSDMS meeting authors template
|CSDMS meeting coauthor first name abstract=Paul
|CSDMS meeting coauthor last name abstract=O'Sullivan
|CSDMS meeting coauthor institute / Organization=GeoSep Services
|CSDMS meeting coauthor town-city=Moscow
|CSDMS meeting coauthor country=United States
|State=Idaho
}}
{{CSDMS meeting abstract template 2023
|CSDMS meeting abstract=Landscapes are sensitive recorders of deep Earth processes that we cannot otherwise directly observe and can provide critical constraints on the geodynamic processes involved in subduction zone orogenesis. Here, we recover continuous 30 Myr rock uplift histories for three bedrock catchments in the forearc above the Calabrian subduction zone, a classic example of a retreating subduction system in southern Italy. Construction of the long-term rock uplift record is enabled by a novel data-driven inversion of tectonic geomorphology measurements, which include low-temperature thermochronology, cosmogenic radionuclides, marine terraces, and fluvial topography. Rock uplift histories from all catchments are similar, exhibiting high rates (>1 mm/yr) from ~30 – 25 Ma that progressively decline to <0.4 mm/yr by ~15 Ma and stay low before abruptly increasing to ~0.65 mm/yr at ~1.5 – 1.0 Ma. The rock uplift results bear little resemblance to the subduction velocity history, implying that crustal thickening through changes in accretionary flux does not dominate uplift during the subduction history. Through comparisons with slab descent reconstructions, we argue that the forearc uplift history primarily reflects the progressive establishment and abrupt destruction of an upper mantle convection cell with strong negative buoyancy beneath the forearc. As the slab freely descended through the upper mantle, the size and vigor of the convection cell grew, slowly drawing forward rock uplift rates down from ~25 – 15 Ma. Once the slab encountered the 660 km mantle transition zone, the convection cell was fully established, subduing uplift rates before slab fragmentation and associated small-scale mantle flow disrupted this condition in the Quaternary, facilitating rapid forearc rock uplift.
}}
}}
{{CSDMS meeting abstract poster Epub 2023}}
{{CSDMS meeting abstract title temp2023}}
{{CSDMS meeting abstract template 2023}}
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Latest revision as of 09:17, 19 April 2023



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Joe Hughes (he/him) choose to not submit an abstract for this conference.