150 research outputs found

    The effects of Venus' thermal structure on buoyant magma ascent

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    The recent Magellan images have revealed a broad spatial distribution of surface volcanism on Venus. Previous work in modeling the ascent of magma on both Venus and Earth has indicated that the planetary thermal structure significantly influences the magmatic cooling rates and thus the amount of magma that can be transported to the surface before solidification. In order to understand which aspects of the thermal structure have the greatest influence on the cooling of ascending magma, we have constructed magma cooling curves for both plutonic and crack buoyant ascent mechanisms, and evaluated the curves for variations in the planetary mantle temperature, thermal gradient curvature with depth, surface temperature gradient, and surface temperature. The planetary thermal structure is modeled as T/T(sub 0) = 1-tau(1-Z/Z(sub 0)(exp n), where T is the temperature, T(sub 0) is the source depth temperature, tau = 1-(T(sub s)/T(sub 0)) where T(sub s) is the planetary surface temperature, Z is the depth, Z(sub 0) is the source depth, and n is a constant that controls thermal gradient curvature with depth. The equation is used both for mathematical convenience and flexibility, as well as its fit to the thermal gradients predicted by the cooling half-space models. We assume a constant velocity buoyant ascent, body-averaged magma temperatures and properties, an initially crystal-free magma, and the same liquidus and solidus for both Venus and Earth

    Gate-to-Gate Life-Cycle Inventory of Softwood Plywood Production

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    A life-cycle inventory (LCI) study is conducted of softwood plywood manufacturing. This gate-to-gate study includes all materials, fuels, and electricity inputs to produce plywood, co-products and emissions. Data were collected through surveys of manufacturing facilities in the Pacific Northwest and the Southeast. SimaPro software, a program to conduct life-cycle inventory studies, is used to process the data and determine environmental impacts in terms of material use and emissions. The data are allocated on a mass basis to plywood based on their contribution to the mass sum of all product and co-products. All data are provided on a production unit basis of 1.0 m3 and 1.0 MSF 3/8-inch basis, the U.S. industry standard. In addition to LCI data, carbon flow data are also given. The LCI data are publicly available through reports, this publication, and the U.S. LCI Database Project. The data are useful for generating cradle-to-gate product LCIs when combined with the LCIs to produce logs for the mills and material transportation impacts, and are useful as a benchmark for assessing process performance, for conducting life-cycle analysis of wall, floor, and roof assemblies consisting of plywood and other products, and of residential structures

    Spatial and Alignment Analyses for a field of Small Volcanic Vents South of Pavonis Mons Mars

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    The Tharsis province of Mars displays a variety of small volcanic vent (10s krn in diameter) morphologies. These features were identified in Mariner and Viking images [1-4], and Mars Orbiter Laser Altimeter (MOLA) data show them to be more abundant than originally observed [5,6]. Recent studies are classifying their diverse morphologies [7-9]. Building on this work, we are mapping the location of small volcanic vents (small-vents) in the Tharsis province using MOLA, Thermal Emission Imaging System, and High Resolution Stereo Camera data [10]. Here we report on a preliminary study of the spatial and alignment relationships between small-vents south of Pavonis Mons, as determined by nearest neighbor and two-point azimuth statistical analyses. Terrestrial monogenetic volcanic fields display four fundamental characteristics: 1) recurrence rates of eruptions,2 ) vent abundance, 3) vent distribution, and 4) tectonic relationships [11]. While understanding recurrence rates typically requires field measurements, insight into vent abundance, distribution, and tectonic relationships can be established by mapping of remotely sensed data, and subsequent application of spatial statistical studies [11,12], the goal of which is to link the distribution of vents to causal processes
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