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Dive into the research topics where Emily M. Taylor is active.

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Featured researches published by Emily M. Taylor.


Quaternary Research | 1983

A Quantitative Comparison of Soil Development in Four Climatic Regimes

Jennifer W. Harden; Emily M. Taylor

Abstract A new quantitative Soil Development Index based on field data has been applied to chronosequences formed under different climatic regimes. The four soil chronosequences, developed primarily on sandy deposits, have some numeric age control and are located in xeric-inland (Merced, Calif.), xeric-coastal (Ventura, Calif.), aridic (Las Cruces, N. Mex.), and udic (Susquehanna Valley, Pa.) soil-moisture regimes. To quantify field properties, points are assigned for developmental increases in soil properties in comparison to the parent material. Currently ten soil-field properties are quantified and normalized for each horizon in a given chronosequence, including two new properties for carbonate-rich soils in addition to the eight properties previously defined. When individual properties or the combined indexes are plotted as a function of numeric age, rates of soil development can be compared in different climates. The results demonstrate that (1) the Soil Development Index can be applied to very different soil types, (2) many field properties develop systematically in different climatic regimes, (3) certain properties appear to have similar rates of development in different climates, and (4) the Profile Index that combines different field properties increases significantly with age and appears to develop at similar rates in different climates. The Soil Development Index can serve as a preliminary guide to soil age where other age control is lacking and can be used to correlate deposits of different geographical and climatic regions.


Geological Society of America Bulletin | 1995

Quaternary soils and dust deposition in southern Nevada and California

Marith C. Reheis; Jonathan C. Goodmacher; Jennifer W. Harden; Leslie D. McFadden; Thomas K. Rockwell; Ralph R. Shroba; Janet M. Sowers; Emily M. Taylor

Eoliandustconstitutesmuchofthepedogenic material in late Pleistocene and Holocene soils of many arid regions of the world.Comparisonofthecompositionsand influx rates of modern dust with the eolian component of dated soils at 24 sites in southern Nevada and California yields informationon(1)thecompositionandinflux rate of dust in late Pleistocene and Holocene soils, (2) paleoclimate and its effects on the genesis of aridic soils, especially with regard to dustfall events, (3) the timing and relative contribution of dust from playa sources versus alluvial sources, and (4) the effects of accumulation of dust in soil horizons. The<2mmfractionsofAandBhorizons of soils formed on gravelly alluvial-fan deposits in the study area are similar to moderndustingrainsize,contentofCaCO3and salt,majoroxides,andclaymineralogy;thus, they are interpreted to consist largely of dust. The major-oxide compositions of the shallow soil horizons are nearly identical to that of the modern dust, but the compositions of progressively deeper horizons approachthatoftheparentmaterial.Theclay mineralogyofmoderndustatagivensiteis similar to that of the Av horizons of nearby Holocene soils but is commonly different from the mineralogies of deeper soil horizonsandoftheAvhorizonsofnearbyPleistocenesoils.Theseresultsareinterpretedto indicate that dust both accumulates and is transformed in Av horizons with time. Changes in soil-accumulation rates provide insights into the interplay of paleoclimate,dustsupply,andsoil-formingprocesses. Modern dust-deposition rates are more than large enough to account for middle and late Holocene soil-accumulation rates at nearly all sites. However, the early Holocene soil-accumulation rates in areas near late Pleistocene pluvial lakes are much higher than modern rates and clearly indicate a dust-deflation and -deposition event that caused rapid formation offine-grained shallow soil horizons on uppermost Pleistocene and lower Holocene deposits. We interpret late Pleistocene soil-accumulation rates to indicate that dust-deposition rates were low during this period but that increased effective moisture during the late Wisconsinan favored translocation of clay andCaCO3fromnearthesurfacetodeeper inthesoilprofile.Pre‐latePleistocenerates are very low in most areas, mainly due to a pedogenic threshold that was crossed when accumulations of silt, clay, and CaCO3 began to inhibit the downward transport of eolian material, but in part due to erosion.


Geoderma | 1992

Morphology and genesis of carbonate soils on the Kyle Canyon fan, Nevada, U.S.A.

Marith C. Reheis; Janet M. Sowers; Emily M. Taylor; Leslie D. McFadden; Jennifer W. Harden

The physical and chemical properties of soils formed in an arid climate on calcareous alluvium of the Kyle Canyon alluvial fan, southern Nevada, were studied in order to infer the rates and relative importance of various soil-forming processes. These studies included field and microscopic observations and analyses of thin sections, major oxides, extractable iron, and clay minerals. The results are interpreted to reflect five major pedogenic processes: (1) The calcic horizons and calcretes of Kyle Canyon soils form by precipitation of CaCO3, derived from eolian dust and alluvium, as clast coats, matrix cement, and massive layers. (2) The A and uppermost B horizons are essentially dust-derived, for they contain large amounts of detrital material not present in the alluvial parent material, and their major-oxide content is similar to that of modern dust. (3) Clay particles are translocated from A into B horizons. (4) Iron-bearing minerals in the near-surface B horizons are slowly oxidized. (5) Carbonate and aluminosilicate grains are both displaced and replaced by pedogenic CaCO3; the silica released by replacement of aluminosilicates may be locally precipitated as amorphous or opaline silica and (or) incorporated into newly formed palygorskite and sepiolite. Rates of soil development at Kyle Canyon are approximate due to uncertainties in age estimates. Some soil field properties change at rates that are similar to rates for soils formed in rhyolitic parent material near Mercury, Nevada. The rate of accumulation of CaCO3 (3–5 g m−2 yr−1) at Kyle Canyon is an order of magnitude faster than that near Mercury, but is comparable to rates calculated for soils in southern New Mexico and Utah.


Quaternary Research | 1991

Rates of soil development from four soil chronosequences in the southern Great Basin

Jennifer W. Harden; Emily M. Taylor; Cindy Hill; Robert K. Mark; Leslie D. McFadden; Marith C. Reheis; Janet M. Sowers; Steven G. Wells

Abstract Four soil chronosequences in the southern Great Basin were examined in order to study and quantify soil development during the Quaternary. Soils of all four areas are developed in gravelly alluvial fans in semiarid climates with 8 to 40 cm mean annual precipitation. Lithologies of alluvium are granite-gneiss at Silver Lake, granite and basalt at Cima Volcanic Field, limestone at Kyle Canyon, and siliceous volcanic rocks at Fortymile Wash. Ages of the soils are approximated from several radiometric and experimental techniques, and rates are assessed using a conservative mathematical approach. Average rates for Holocene soils at Silver Lake are about 10 times higher than for Pleistocene soils at Kyle Canyon and Fortymile Wash, based on limited age control. Holocene soils in all four areas appear to develop at similar rates, and Pleistocene soils at Kyle Canyon and Fortymile Wash may differ by only a factor of 2 to 4. Over time spans of several millennia, a preferred model for the age curves is not linear but may be exponential or parabolic, in which rates decrease with increasing age. These preliminary results imply that the geographical variation in rates within the southern Great Basin-Mojave region may be much less significant than temporal variation in rates of soil development. The reasons for temporal variation in rates and processes of soil development are complexly linked to climatic change and related changes in water and dust, erosional history, and internally driven chemical and physical processes.


Geosphere | 2010

Three-dimensional geologic modeling of the Santa Rosa Plain, California

Donald S. Sweetkind; Emily M. Taylor; Craig A. McCabe; V.E. Langenheim; Robert J. McLaughlin

New three-dimensional (3D) lithologic and stratigraphic models of the Santa Rosa Plain (California, USA) delineate the thickness, extent, and distribution of subsurface geologic units and allow integration of diverse data sets to produce a lithologic, stratigraphic, and structural architecture for the region. This framework can be used to predict pathways of groundwater flow beneath the Santa Rosa Plain and potential areas of enhanced or focused seismic shaking. Lithologic descriptions from 2683 wells were simplified to 19 internally consistent lithologic classes. These distinctive lithologic classes were used to construct a 3D model of lithologic variations within the basin by extrapolating data away from drill holes using a nearest-neighbor approach. Subsurface stratigraphy was defined through the identification of distinctive lithologic packages tied, where possible, to high-quality well control and to surface exposures. The 3D stratigraphic model consists of three bounding components: fault surfaces, stratigraphic surfaces, and a surface representing the top of pre-Cenozoic basement, derived from inversion of regional gravity data. The 3D lithologic model displays a west to east transition from dominantly marine sands to heterogeneous continental sediments. In contrast to previous stratigraphic studies, the new models emphasize the prevalence of the clay-rich Petaluma Formation and its heterogeneous nature. Isopach maps of the Glen Ellen Formation and the 3D stratigraphic model show the influence of the Trenton Ridge, a concealed basement ridge that bisects the plain, on sedimentation; the thickest deposits of the Glen Ellen Formation are confined to north of the Trenton Ridge.


Scientific Investigations Map | 2014

Quaternary geologic map of the north-central part of the Salinas River Valley and Arroyo Seco, Monterey County, California

Emily M. Taylor; Donald S. Sweetkind

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IMAP | 2002

Geologic map of the Yucca Mountain region, Nye County, Nevada

Christopher J. Potter; R.P. Dickerson; Donald S. Sweetkind; Ronald M. Drake; Emily M. Taylor; Christopher J. Fridrich; Carma A. San Juan; Warren C. Day


Scientific Investigations Report | 2014

Three-dimensional geologic mapping of the Cenozoic basin fill, Amargosa Desert basin, Nevada and California

Emily M. Taylor; Donald S. Sweetkind


Archive | 2008

Plio-Pleistocene Evolution of Concealed Basins Separated by a Bedrock Ridge West of the Rodgers Creek and Healdsburg Faults, Northern California

Donald S. Sweetkind; Robert J. McLaughlin; V. E. Langenheim; Richard A. J. Williams; Emily M. Taylor; Darcy K. McPhee; David B. Wahl; Andrei M. Sarna-Wojcicki; Robert McKee; Kerry Locke


Scientific Investigations Map | 2017

Surficial geologic map of Berrien County, Michigan, and the adjacent offshore area of Lake Michigan

Byron D. Stone; Kevin A. Kincare; Dennis W. O'Leary; Wayne L. Newell; Emily M. Taylor; Van S. Williams; Scott C. Lundstrom; Jared E. Abraham; Michael H. Powers

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Donald S. Sweetkind

United States Geological Survey

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Jennifer W. Harden

United States Geological Survey

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Marith C. Reheis

United States Geological Survey

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Christopher J. Fridrich

United States Geological Survey

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Robert J. McLaughlin

United States Geological Survey

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Andrei M. Sarna-Wojcicki

United States Geological Survey

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Byron D. Stone

United States Geological Survey

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