1 dsolproc.doc 5/1/95 SAMPLING AND LABORATORY PROCEDURES AND MATHEMATICAL EQUATIONS FOR SOILS AT DUST-TRAP SITES IN SOUTHERN NEVADA AND CALIFORNIA file dsolloc.xls Named soil localities in this file are taken from previously published studies at sites where we had placed dust traps in 1984. Numbered soil localities correspond to dust-trap sites where soils were described and sampled after the traps were in place, mainly in 1988 and 1989. References cited in the file are listed at the end of this document. file dsoldes.xls Numbered profiles (11H, 11P, etc.) were sampled specifically for this study. Two profiles from San Felipe Creek (SF1 and SF3) are unpublished data contributed by Tom Rockwell (San Diego State University). Methods for the descriptions of all of the soils were the same. Soil profiles were described and sampled in many places where no previous soil studies had been done. In each area, two alluvial-fan surfaces were selected that were thought to be late Pleistocene and middle to late Holocene in age by comparison of surface characteristics such as pavement, varnish, and preservation of depositional topography to those of dated surfaces from previous studies in the region (for example, McFadden and others, 1989; Reheis and others, 1993.i.Reheis, 1992;). One soil profile was described and sampled on each surface using either fresh stream cuts or hand-dug pits. Soil descriptions and horizon names followed Guthrie and Witty (1982) and Birkeland (1984). Stages of CaCO3 , silica, and salt follow definitions of Gile and others (1966), Taylor (1986), and Reheis (1987), respectively. file dsindprn.xls The soil development index (Harden, 1982) provides a means of quantifying field properties of soils in order to compare their development. Index values of field properties including rubification, melanization, paling, lightening, texture, structure, dry consistence, pH decrease, pH increase, and carbonate (Harden, 1982; Reheis, 1987; Harden and others, 1991b) are calculated for each profile using a spreadsheet template (Taylor, 1988). Normalized values of these properties are multiplied by horizon thickness to obtain the horizon index; the horizon values within a profile are summed to obtain the profile index. Horizon and profile index values are given for all of the soils sampled for this study. The ages of the soils sampled for this study (11H, 11P, etc.) were estimated from field morphologic data using the soil development index. The index values were compared with values for soils of known age that formed under similar conditions of climate and, where possible, parent material (Taylor, 1986.i.Taylor, 1986;; Reheis and others, 1989.i.Reheis and others, 1989;, 1992.i.Reheis and others, 1992;; Harden and others, 1991a; Slate, 1992.i.Slate, 1992;), and "best" ages and age ranges were assigned to the soil profiles. Harden and others (1991b).i.Harden and others (1991);, using a statistically based version of this technique in a study of soil chronosequences in the southern Great Basin (some of the sites used in this study), suggested that average rates of most soil-development parameters within this area are precise to about a factor of two and that, at least for Holocene soils, estimated ages derived from these rates might be accurate within about a factor of two or three. Sites that provided soil ages for the study were the Whipple Mountains (McFadden, 1982), the Fortymile Wash-Yucca Wash area (henceforth referred to as the Fortymile Wash area; Taylor, 1986), Silver Lake (Reheis and others, 1989), Kyle Canyon (Sowers and others, 1988), the Cima fans (Harden and others, 1991b), Wilson Creek (Harden and Matti, 1989), and the Coyote Mountains (Goodmacher and Rockwell, 1990). Some ages were based on various methods of radiometric dating of deposits and soils, and others were based on correlation of soil properties to those of soils at other dated sites using the soil development index of Harden (1982).i.Harden (1982); and modifications to the index (Reheis, 1987; Taylor, 1988; Harden and others, 1991b). file dsolab.xls Most of the samples were analyzed using standard laboratory techniques (Singer and Janitzky, 1986.i.Singer and Janitzky, 1986;) for grain size, CaCO3 and organic-matter content, pH, and salt content, except that the total salt equations in Singer and Janitzky, published with an error, were corrected using a multiplication factor of 0.32 rather than 320. pH for the soils sampled specifically for this study was measured in 1:1 H2O, whereas the pH for soils from other sources was measured using CaCl2. Some other analytical techniques for the Kyle Canyon soils were also different because the soils formed in carbonate-rich alluvium. The contents of CaCO3 and silt plus clay reported in this table were measured using a combination of chemical, microscopic, and photographic techniques (Sowers, 1988; Reheis et al., 1992) and are the amounts of pedogenic (non-parent material) carbonate and silt plus clay, not total amounts. In addition, the salt content reported for Kyle Canyon soils is for gypsum only, not total salt. Data for Wilson Creek (WC) soils is unpublished data of J.W. Harden; data for Cima fan soils (CV) is unpublished data of E.M. Taylor, J.W. Harden, and L.D. McFadden; data for Silver Lake (SL) soils is unpublished data of M.C. Reheis, J.W. Harden, and L.D. McFadden; data for Kyle Canyon (KC) soils is from Reheis and others (1992); and data for Coyote Mountains (FC and AC) soils is unpublished data of Jonathan Goodmacher (also Goodmacher and Rockwell, 1990) except that salt values are different owing to an error in the original calculations (see first sentence of this section). file dsolpw.xls The bulk density for each soil horizon, if not measured by previous reports using either the paraffin-clod method or the excavation technique, was estimated from particle size and the contents of gravel and organic matter using the technique of Rawls (1983).i.Rawls (1983);. Profile weights (g/cm2/soil column) were calculated for pedogenic silt, clay, CaCO3, and salt (where possible). The contents (percentages) of these components in each horizon of a soil were subtracted from the contents estimated to have been present in the parent material (method of Machette, 1985), multiplied by the bulk density of the less-than-2mm fraction and by horizon thickness, and then summed for the soil. At most sites, the parent material consisted of alluvial-fan deposits, commonly debris flows. Debris flows are usually unsorted and unbedded, so the content of silt, clay, and CaCO3 in a C horizon formed in these deposits was assumed to be representative of that originally present in the other horizons. For soils at Wilson Creek that formed in fluvial deposits potentially containing fine-grained overbank sediment (Harden and Matti, 1989), amounts of silt and clay in the parent material of the A and B horizons were estimated to be greater than those in the C horizons. Basalt flows were assumed to contain no silt, clay, or CaCO3 when deposited. In this study, we assume that the dust component of soils is pedogenic, not parent material, and that all silt, clay, and CaCO3 present in greater proportions in a soil than in the parent material is pedogenic material and ultimately derived from dust. Soils that formed in carbonate alluvium are one exception; they contain abundant CaCO3 derived from solution of the parent material (Sowers, 1985; Reheis and others, 1992). The major-oxide composition and clay mineralogy of the dust and soil horizons support this assumption. Previous work in the study area (McFadden, 1982; McFadden and others, 1986; Taylor, 1986; Reheis and others, 1989, 1992) indicated little chemical weathering in soils of this age. Soils that are more than about 100,000 years old or that formed in semiarid to subhumid climates have likely been chemically weathered. However, much of the silt, clay, and CaCO3 in older aridic soils is likely to be of eolian origin, in part transformed into other minerals or grain sizes by chemical or physical processes. Profile weights for Coyote Mountains soils (AC and FC) were recalculated from original data because profile weights given in Goodmacher and Rockwell (1990) did not account for parent-material values. file dsolox.xls Major-element contents for the Kyle Canyon and Silver Lake soils were measured using wavelength-dispersive X-ray fluorescence spectroscopy (XRF) and zirconium content using energy-dispersive XRF (Baedecker, 1987) on the less-than-2mm fraction including CaCO3. Oxide percentages were recalculated to 100% to correct for the amount of water and other volatiles not measured. For the Wilson Creek soils, only Fe2O3, K2O, CaO, TiO2, MnO, and ZrO2 were measured using energy-dispersive XRF. In order to compare the soil analyses with those of nearby dust samples, which did not include Ca from CaCO3, the contents of major oxides in the soil samples from Kyle Canyon and Silver Lake were recalculated on a CaCO3-free basis (Wilson Creek soils contained no CaCO3). Values for Silver Lake (SL) soils are unpublished data of M.C. Reheis; values for Kyle Canyon soils are from Reheis and others (1992); and values for Wilson Creek (WC) soils are unpublished data of J.W. Harden. file dsolmin.xls The clay mineralogy of soils from published sources was compared to that of modern dust at the same sites (see datafile "dustmin.xls"). Observed differences between the clay mineralogy of soils and dust at some sites are attributed either to clay formation within the soils, to variability not explored sufficiently because too few samples were analyzed, or to slightly different analytical procedures used for the soil and dust samples (different ion saturations, etc.). In addition, the published reports used different methods to estimate abundances of clay minerals from peak heights on X-ray diffraction traces. Soils at Silver Lake were analyzed, and relative abundances of clay minerals estimated, using the same techniques used for the dust samples. Values for Whipple Mountains soils are from McFadden (1982); values for Silver Lake soils are unpublished data of M.C. Reheis; values for Fortymile Wash soils are from Taylor (1986); values for the Mormon Mesa calcrete are from Gardner (1972); values for the Cima volcanic field soils are from McFadden et al., 1986); and values for the Kyle Canyon soils are from Amundson et al. (1989). file averate.xls Accumulation rates were calculated for pedogenic silt, clay, CaCO3, and salt depending on the availability of data. At sites with more than one analyzed soil profile of the same age, the profile-weight values were averaged. The average "best" accumulation rates were calculated using the "best" age (the most reasonable age assigned to the geomorphic surface), and average maximum and minimum rates were calculated using the likely minimum and maximum ages respectively. The following are example calculations for the silt accumulation rate of soils on surface Q5, Coyote Mountains, where the average profile weight of silt in Q5 soils is 0.8 g/cm2, the "best" age is 12 ka, the minimum age is 9 ka, and the maximum age is 20 ka: average "best" accumulation rate = 0.8 g/cm2 / 12,000 yr = 0.7 g/m2/yr average maximum accum. rate = 0.8 g/cm2 / 9,000 yr = 0.9 g/m2/yr average minimum accum. rate = 0.8 g/cm2 / 20,000 yr = 0.4 g/m2/yr file intrate.xls The interval-accumulation rate for each profile is the rate of accumulation of a pedogenic component in a soil forming on a surface from the time of deposition of that surface to the time of deposition of the next younger surface. If there is no younger profile, the interval rate is the same as the average rate. Interval age is the period of time between the formation of one surface and the formation of the next younger surface. Best interval age = best age (older) - best age (younger). Minimum interval age = minimum age (older) - maximum age (younger). Maximum interval age = maximum age (older) - minimum age (younger). As an example, the "best" interval accumulation rate between soils formed on surfaces Q5 and Q4 of the Coyote Mountains, where the average profile weight of silt in Q4 soils is 0.4 g/cm2 and the "best" age is 3 ka is calculated by: interval accum. rate = (0.8 g/cm2 - 0.4 g/cm2) / (12,000 - 3,000 yr) = 0.4 g/m2/yr The interval-rate value is plotted at the midpoint between the two "best" ages, or at 7,500 years. Soil accumulation rates must be treated with caution. (1) Variation in amount of a pedogenic material is expectable for soils of the same age because soils are inherently variable. Data from more than one profile per geomorphic surface is critical for quantitative soil studies (e.g. data for field properties of soils at Silver Lake; Reheis and others, 1989). Standard deviations were only calculated for the interval rates at the Fortymile Wash area, Silver Lake, the Cima fans, Wilson Creek, and the Coyote Mountains, which had quantitative data for more than one profile per surface (file "intrtdev.xls"). Excluding soils that were strongly eroded or leached, the standard deviations average 75% of the rates, but range widely (5-200%). (2) There are uncertainties in the assigned ages of the geomorphic surfaces and their soils. This problem is most acute for the youngest deposits; for example, if a deposit is thought to be 200 years old but in fact is 400 years old, an error of only 200 years would yield a doubled accumulation rate. In addition, radiometric ages are available only for soils from Silver Lake, the Fortymile Wash area, Kyle Canyon, and the Coyote Mountains. We have not included age uncertainties in the calculation of interval rates because generally the minimum and maximum ages greatly exaggerate the probable errors. For studies in which the ages of soils were better constrained, as at Silver Lake and Fortymile Wash, interval-rate uncertainties calculated from the minimum and maximum soil ages were similar to the range of standard deviations calculated using replicate soils of the same age. (3) Assumptions and simplifications were used in the calculations of profile weights of pedogenic materials, mainly in the estimation of parent-material values and of bulk density (in this study, a range of 1.2-2.0 g/cm3), which is difficult to measure accurately in gravelly deposits (Vincent and Chadwick, 1994). file intrtdev.xls Averages and standard deviations were computed for the "best" interval-accumulation rates for sites that had data for more than one soil profile of the same age. Calculations followed the same procedures described in file "intrate.xls" except that to obtain the interval mass, the average interval mass of a younger group of soils was subtracted from the individual interval mass of the next older soil or soils. REFERENCES Amundson, R.G., Chadwick, O.A., Sowers, J.M., and Doner, H.E., 1989, Soil evolution along an altitudinal transect in the eastern Mojave Desert of Nevada, U.S.A.: Geoderma, v. 43, p. 349-371. Baedecker, P.A., 1987, ed., Methods for Geochemical Analysis: U.S. Geological Survey Bulletin 1770. Birkeland, P.W., 1984, Soils and Geomorphology: New York, Oxford University Press, 372 p. Gardner, L.R., 1972, Origin of the Mormon Mesa caliche, Clark County, Nevada: Geological Society of America Bulletin, v. 83, p. 143-156. Gile, L.H., Peterson, F.F., and Grossman, R.B., 1966, Morphological and genetic sequences of carbonate accumulation in desert soils: Soil Science, v. 99, p. 74-82. Goodmacher, J., and Rockwell, T., 1990, Properties and inferred ages of soils developed in alluvial deposits in the southwestern Coyote Mountains, Imperial County, California, in Rockwell, T. R., ed., Friends of the Pleistocene, Winter Fieldtrip-1990, Western Salton Trough Soils and Neotectonics: San Diego, California, Privately published, p. 43-104. Guthrie, R.L., and Witty, J.E., 1982, New designations for soil horizons and layers and a new soil survey manual: Soil Sci. Soc. Amer. 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Taylor, E.M., 1986, Impact of time and climate on Quaternary soils in the Yucca Mountain area of the Nevada Test Site: M.S. thesis, University of Colorado, Boulder, 217 p. ---, 1988, Instructions for the soil development index template--LOTUS 1-2-3 (and program disk): U.S. Geological Survey Open-File Report 88-233, 23 p. Vincent, K.R., and Chadwick, O.A., 1994, Synthesizing bulk density for soils with abundant rock fragments: Soil Science Society of America Journal, v. 58, p. 455-464.