Windblown sand on Venus: Preliminary results of laboratory simulations     

R. Greeley  J. Iversen  R. Leach  J. Marshall  B. White  S. Williams 《Icarus》1984,57(1):112-124

Small particles and winds of sufficient strength to move them have been detected from Venera and Pioneer-Venus data and suggest the existence of aeolian processes on Venus. The Venus wind tunnel (VWT) was fabricated in order to investigate the behavior of windblown particles in a simulated Venusian environment. Preliminary results show that sand-size material is readily entrained at the wind speeds detected on Venus and that saltating grains achieve velocities closely matching those of the wind. Measurements of saltation threshold and particle flux for various particle sizes have been compared with theoretical models which were developed by extrapolation of findings from Martian and terrestial simulations. Results are in general agreement with theory, although certain discrepancies are apparent which may be attributed to experimental and/or theoretical-modeling procedures. Present findings enable a better understanding of Venusian surface processes and suggest that aeolian processes are important in the geological evolution of Venus.  相似文献   

Ultraviolet spectroscopic determination of the stability constants for copper carbonate and bicarbonate complexes up to the ionic strength of seawater     

Richard W Zuehlke  Dana R Kester 《Marine Chemistry》1983,13(3):203-226

An ultraviolet spectroscopic study at 25°C is used to determine the stoichiometric stability constant of CuCO₃⁰ (β_CuCO3⁰) over a range of ionic strengths; extrapolation to zero ionic strength provides a thermodynamic constant (log β⁰_CuCO3⁰ = 6.89). At 0.69 m ionic strength, log β_CuCO3⁰) is 6.33.This study provides the first experimental evidence for the existence of CuHCO₃⁺. At 0.69 m ionic strength, log β_CuHCO3⁺ is 2.77.The ultraviolet molal absorptivity spectra for the two complexes are also determined. The spectrum for CuCO₃⁰ consists of a single band centered at 276.5 nm and was described well by a Gaussian function. The spectrum of CuHCO₃⁺ consists of at least two overlapping bands.Side reactions which might affect the data interpretation were included in the analysis of the results. The effects of the Cu(II) hydrolysis reactions were accounted for by using data from previous work, and possible effects due to copper-organic species were eliminated by a subtraction procedure.  相似文献   

Constraints on clinopyroxene/melt partitioning of REE, Rb, Sr, Ti, Cr, Zr, and Nb during mantle melting: First insights from direct peridotite melting experiments at 1.0 GPa     

A. Dana Johnston  Brandon E. Schwab 《Geochimica et cosmochimica acta》2004,68(23):4949-4962

Earlier piston-cylinder experiments in our laboratory produced a collection of mantle melting run products at 1.0 GPa that have now been analyzed by ion probe for selected REE, Ti, Cr, Rb, Sr, Y, Zr, and Nb. Natural starting materials were used and experiments were run in graphite-lined Pt capsules with the melt separated from the residual minerals into a layer of vitreous carbon spheres (VCS) to circumvent quench modification. The glass phase in 18 run products, representing melt percentages of ∼2-20 wt%, yielded excellent data that were inverted to yield the first estimates ever of clinopyroxene/melt distribution coefficients, Ds, derived from direct peridotite partial melting experiments. Uncertainties were estimated with a Monte Carlo method.For the REE and Y, these Ds were then compared to Ds calculated with the widely-used model of Wood and Blundy (1997) and the two sets overlap at the ±2σ level in 123 of 128 cases (∼96%). This indicates to us that: 1) the experiments analyzed here are well equilibrated with respect to major and trace element distributions, thus supporting the efficacy of the VCS technique and its variation involving diamond (e.g., Baker and Stolper, “Determining the composition of high-pressure mantle melts using diamond aggregates” [1994], Geochim. Cosmochim. Acta58, 2811-2827); 2) the model of Wood and Blundy (1997), calibrated largely on the basis of large melt fraction, inverse- or sandwich-type experiments, describes REE and Y partitioning during peridotite melting well, even very near the solidus; and it suggests that the cpx/melt Ds derived here for other elements, not modeled by the Wood and Blundy formulation, are probably also correct for peridotite melting to within their ±2σ uncertainties. D^sp/liq and D^cpx/liq values for Cr calculated directly from electron microprobe data decrease by about a factor of five with increasing temperature and melt percentage.The degree to which our experiments appear to have equilibrated seems at odds with recent measurements of the diffusivities of REE in diopside which suggest that relatively small percentages of our starting mineral grains should have equilibrated diffusively. Instead, we suggest that equilibration occurs much more rapidly through the processes of recrystallization and grain coarsening, accomplished through dissolution and reprecipitation. This suggestion is supported by the observation that our final grain sizes are typically 5-10 times larger than the ∼10 μm starting sizes, indicating that substantial mass transfer occurred in our experiments, probably mediated by the melt phase in which diffusion is faster.  相似文献   

Constraints from Moho geometry and crustal thickness on the geodynamic origin of the Vrancea Seismogenic Zone (Romania)     

Dana M. Mucuta  Camelia C. Knapp  James H. Knapp 《Tectonophysics》2006,420(1-2):23

Reprocessing of industry deep seismic reflection data (Ramnicu Sarat and Braila profiles) from the SE Carpathian foreland of Romania provides important new constraints on geodynamic models for the origin of the intermediate depth Vrancea Seismogenic Zone (VSZ). Mantle (70–200 km) earthquakes of the VSZ are characterized by high magnitudes (greater than 6.5), frequent occurrence rates (approximately 25 years), and confinement in a very narrow (30 × 70 × 200 km³) near vertical zone atypical for a Wadati–Benioff plane, located in front of the orogen. These two deep (20 s) seismic reflection profiles (70 km length across the foreland) reveal (1) a high-amplitude, gently east-dipping reflection across most of the section from what we interpret to be the Moho at  15 s (40–42 km) on the Ramnicu Sarat line to  16 s (47–48 km) on the Braila line, (2) a thick sedimentary cover increasing in thickness from east (1 s;  800 m) to west (7.5 s; 14 km), (3) an eastward increase in crustal thickness from 38 km (near VSZ) to  45 km, (4) seismic and topographic evidence for a newly imaged, possibly seismically active basement fault with a surface offset of 30 m observed on the Ramnicu Sarat line, (5) a lack of notable west-dipping structures in the crust and across the Moho, and (6) variable displacements on Peceneaga–Camena Fault of  5 km at Moho and  200 m at the basement–sedimentary cover contact.These observations appear to argue against recent models for west-dipping subduction of oceanic lithosphere at or in the vicinity of the Vrancea Seismogenic Zone given the lack of west-dipping fabrics in the lower crust and across the crust–mantle boundary. Consequently, one possible explanation for the geodynamic origin of VSZ could be partial delamination of the continental lithosphere in an intra-plate setting along a sub-horizontal lithospheric interface in the Carpathian hinterland that likely involves remnant lithospheric coupling between the crust and uppermost mantle in the foreland.  相似文献   

Snow pack in the Romanian Carpathians under changing climatic conditions   总被引：2，自引：0，他引：2  

Dana Micu 《Meteorology and Atmospheric Physics》2009,105(1-2):1-16

Snow pack characteristics and duration are considered to be key indicators of climate change in mountain regions, especially during the winter season (herein considered to last from the 1st of November to the 30th of April). Deviations recorded in the regime of the main explanatory variables of snow pack changes (i.e. temperature and precipitation) offer useful information on winter climate variability, in the conditions of the winter warming trend already seen in some areas of the Romanian Carpathians. The present work focuses on changes and trends in snow pack characteristics and its related parameters, registered at the 15 weather stations located in the alpine, sub-alpine and forest belts in all the three Romanian Carpathian branches (>1,000 m) over the 1961–2003 period. Changes in the snow pack regime were investigated in relation with the modifications of winter temperature and precipitation having been detected mostly at the end of the twentieth century. A winter standardized index was calculated to group winters over the 43-year period into severity classes and detect the respective changes. Links between the number of snow cover days and seasonal NAO index were also statistically analysed in this study. The general results show large regional and altitudinal variations and the complex character of the climate in the Romanian Carpathians, leading to the idea of an ongoing warming process associated with a lower incidence of snow cover, affecting to a large extent the forested mountain areas located below 1,600–1,700 m altitude. Also negative and weak correlations were found, particularly over the December–March interval, between the number of snow cover days and seasonal NAO index values.  相似文献   

Predictions of Energy and Helicity in Four Major Eruptive Solar Flares   总被引：1，自引：0，他引：1  

Maria D. Kazachenko  Richard C. Canfield  Dana W. Longcope  Jiong Qiu 《Solar physics》2012,277(1):165-183

In order to better understand the solar genesis of interplanetary magnetic clouds (MCs), we model the magnetic and topological properties of four large eruptive solar flares and relate them to observations. We use the three-dimensional Minimum Current Corona model (Longcope, 1996, Solar Phys. 169, 91) and observations of pre-flare photospheric magnetic field and flare ribbons to derive values of reconnected magnetic flux, flare energy, flux rope helicity, and orientation of the flux-rope poloidal field. We compare model predictions of those quantities to flare and MC observations, and within the estimated uncertainties of the methods used find the following: The predicted model reconnection fluxes are equal to or lower than the reconnection fluxes inferred from the observed ribbon motions. Both observed and model reconnection fluxes match the MC poloidal fluxes. The predicted flux-rope helicities match the MC helicities. The predicted free energies lie between the observed energies and the estimated total flare luminosities. The direction of the leading edge of the MC’s poloidal field is aligned with the poloidal field of the flux rope in the AR rather than the global dipole field. These findings compel us to believe that magnetic clouds associated with these four solar flares are formed by low-corona magnetic reconnection during the eruption, rather than eruption of pre-existing structures in the corona or formation in the upper corona with participation of the global magnetic field. We also note that since all four flares occurred in active regions without significant pre-flare flux emergence and cancelation, the energy and helicity that we find are stored by shearing and rotating motions, which are sufficient to account for the observed radiative flare energy and MC helicity.  相似文献   

Evaporation of the Nerve Agent GB From Common Matrices: A Model‐System Study          下载免费PDF全文

Ishay Columbus  Itzhak Marcovitch  Shlomi Elias  Lea Yehezkel  Dana Marder  Victoria Nahum 《洁净——土壤、空气、水》2018,46(4)

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Comparison of surface and borehole locations of induced seismicity   总被引：1，自引：0，他引：1  

Leo Eisner  B. J. Hulsey  Peter Duncan  Dana Jurick  Heigl Werner  William Keller 《Geophysical Prospecting》2010,58(5):809-820

Monitoring of induced microseismic events has become an important tool in hydraulic fracture diagnostics and understanding fractured reservoirs in general. We compare microseismic event and their uncertainties using data sets obtained with surface and downhole arrays of receivers. We first model the uncertainties to understand the effect of different acquisition geometries on location accuracy. For a vertical array of receivers in a single monitoring borehole, we find that the largest part of the final location uncertainty is related to estimation of the backazimuth. This is followed by uncertainty in the vertical position and radial distance from the receivers. For surface monitoring, the largest uncertainty lies in the vertical position due to the use of only a single phase (usually P‐wave) in the estimation of the event location. In surface monitoring results, lateral positions are estimated robustly and are not sensitive to the velocity model. In this case study, we compare event location solutions from two catalogues of microseismic events; one from a downhole array and the second from a surface array of 1C geophone. Our results show that origin time can be reliably used to find matching events between the downhole and surface catalogues. The locations of the corresponding events display a systematic shift consistent with a poorly calibrated velocity model for downhole dataset. For this case study, locations derived from surface monitoring have less scatter in both vertical and horizontal directions.  相似文献   

Variability of stream extents controlled by flow regime and network hydraulic scaling     

Dana A. Lapides  Christine D. Leclerc  Hana Moidu  David N. Dralle  W. Jesse Hahm 《水文研究》2021,35(3):e14079

Stream networks expand and contract through time, impacting chemical export, aquatic habitat, and water quality. Although recent advances improve prediction of the extent of the wetted channel network (L ) based on discharge at the catchment outlet (Q ), controls on the temporal variability of L remain poorly understood and unquantified. Here we develop a quantitative, conceptual framework to explore how flow regime and stream network hydraulic scaling factors co-determine the relative temporal variability in L (denoted here as the total wetted channel drainage density). Network hydraulic scaling determines how much L changes for a change in Q , while the flow regime describes how Q changes in time. We compiled datasets of co-located dynamic stream extent mapping and discharge to analyze all globally available empirical data using the presented framework. We found that although variability in L is universally damped relative to variability in Q (i.e., streamflow is relatively more variable in time than network extent), the relationship is elastic, meaning that for a given increase in the variability in Q , headwater catchments will experience greater-than-proportional increases in the variability of L . Thus, under anticipated climatic shifts towards more volatile precipitation, relative variability in headwater stream network extents can be expected to increase even more than the relative variability of discharge itself. Comparison between network extents inferred from the L -Q relationship and blue lines on USGS topographic maps shows widespread underestimation of the wetted channel network by the blue line network.  相似文献   

The distribution of iron in the Northwest Atlantic     

James L Symes  Dana R Kester 《Marine Chemistry》1985,17(1):57-74

Samples from eleven stations in the Sargasso Sea, Slope Water, and continental shelf water of the Northwest Atlantic have been analyzed for total iron by atomic absorption spectrophotometry. Vertical profiles for iron and associated temperature and nutrient data were obtained at the five open-ocean stations. Data from six stations provided a transect across the continental shelf into the apex of the New York Bight.At open-ocean stations, iron was depleted near the surface to levels of about 1–2 nmol kg^?1 and increased to levels of about 4–7 nmol kg^?1 in the vicinity of the oxygen minimum. A characteristic bottom-water maximum was observed at stations where closely spaced, near-bottom sampling was conducted. This feature was due at least partially to resuspension of particulate iron associated with the nepheloid layer.Comparison of total iron concentrations (available upon digestion in concentrated nitric acid) to those of filtered samples (0.4 μm) at one Slope Water station indicated that about 40% of the available iron in the water column was associated with the particulate phase. Near the surface, in the vicinity of the chlorophyll maximum, iron was present almost totally in particulate form. The dissolved fraction increased to approximately 50% at the nutrient maximum and approached 100% in the mid-portion of the water column. In deeper waters, the particulate fraction again became important, increasing to approximately 80% of the total iron in the near-bottom maximum.In the apex of the New York Bight, iron levels in excess of 200 and 500 nmol kg^?1 were observed in surface and bottom waters, respectively. In the mid-continental shelf region, the iron distribution does not appear to be greatly influenced by coastal sources; within 65 km of the coastline, iron levels approached open-ocean values.  相似文献