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The Fisher Valley basin (FVB), located adjacent to the Onion Creek salt diapir, Paradox basin, Utah, USA, constitutes one of the thickest collections of Quaternary sediments within the Colorado Plateau. These sediments are important for constraining regional paleoclimate environments as well as recent tectonic movement of the Onion Creek salt diapir. Here, we combine magnetic susceptibility data with previously published age constraints (Bishop Tuff and Lava Creek B ash) into a cyclostratigraphic analysis of these sediments. We present a refined and astronomically tuned age model that demonstrates that deposition of the upper basin fill was between ca. 765 ka and 212 ± 8 ka. Correlating this chronologic model to environmental magnetic proxies, we show that from ca. 765 ka to ca. 535 ka, magnetic mineral assemblages deposited during glacials were characterized by generally finer grain sizes (elevated χARM/χlow) than during interglacials. These data are consistent with glacial periods being characterized by either wetter conditions amenable to pedogenesis, or drier conditions associated with increased concentrations of windblown dust. Interglacials are characterized by generally coarser magnetic grain sizes (lower χARM/χlow), consistent with periods of episodic alluvial and colluvial deposition in the FVB. At ca. 535 ka, χARM/χlow reach their lowest value (coarsest magnetic grain size) and then begin a progressive transition to higher values, consistent with a generally fining upward stratigraphic sequence throughout the rest of the section. This transition at ca. 535 ka coincides with a peak in sediment accumulation rate of ∼19 cm/k.y. and is most plausibly linked to halokinetic activity of the nearby Onion Creek salt diapir. Thus, although sediments in the FVB appear to be sensitive to global climate patterns between 765 ka and ca. 535 ka, local tectonic processes appear to episodically obscure this sensitivity. 

Abstract. The upper Paleozoic Cutler Group of southern Utah, USA, is a key sedimentary archive for understanding the Earth-life effects of the planet's last pre-Quaternary icehouse–hothouse state change: the Carboniferous–Permian (C–P) transition, between 304 and 290 million years ago. Within the near-paleoequatorial Cutler Group, this transition corresponds to a large-scale aridification trend, loss of aquatic habitats, and ecological shifts toward more terrestrial biota as recorded by its fossil assemblages. However, fundamental questions persist. (1) Did continental drift or shorter-term changes in glacio-eustasy, potentially driven by orbital (Milankovitch) cycles, influence environmental change at near-equatorial latitudes during the C–P climatic transition? (2) What influence did the C–P climatic transition have on the evolution of terrestrial ecosystems and on the diversity and trophic structures of terrestrial vertebrate communities? The Paleozoic Equatorial Records of Melting Ice Ages (PERMIA) project seeks to resolve these issues in part by studying the Elk Ridge no. 1 (ER-1) core, complemented by outcrop studies. This legacy core, collected in 1981 within what is now Bears Ears National Monument, recovered a significant portion of the Hermosa Group and the overlying lower Cutler Group, making it an ideal archive for studying paleoenvironmental change during the C–P transition. As part of this project, the uppermost ∼ 450 m of the core were temporarily transferred from the Austin Core Repository Center to the Continental Scientific Drilling Facility at the University of Minnesota for splitting, imaging, and scanning for geophysical properties and spectrophotometry. Here we (1) review the history of this legacy core, (2) introduce recently obtained geophysical and lithologic datasets based on newly split and imaged core segments to provide a sedimentological and stratigraphic overview of the Elk Ridge no. 1 core that aligns more accurately with the currently recognized regional lithostratigraphic framework, (3) establish the position of the boundary between the lower Cutler beds and the overlying Cedar Mesa Sandstone in the core, and (4) outline our ongoing research goals for the core. In-progress work on the core aims to refine biostratigraphic and chemostratigraphic age constraints, retrieve the polarity stratigraphy, interrogate preserved cyclostratigraphy, analyze sedimentary structures and paleosol facies, investigate stable isotope geochemistry, and evaluate elemental abundance data from X-ray fluorescence (XRF) scanning. Together with outcrop studies throughout Bears Ears National Monument and its vicinity, these cores will allow the rich paleontological and paleoenvironmental archives recorded in the continental Carboniferous–Permian transition of western North America to be confidently placed in a robust chronologic context that will help test hypotheses relating ecosystem evolution to the Carboniferous rainforest collapse, initial decline of the Late Paleozoic Ice Age, and long-wavelength astronomical cycles pacing global environmental change.