A Causal Model of Individual Decision Making Under Time Pressure

In Figure 1 we present a causal model of the relationship between time pressure and decision quality.The model represents causes and effects in an individual actor working toward a decision. This model distinguishes between the actor\u27s perception of high effort per unit time and the psychological stress that may result from such a perception. An explanation of the model is followed by recommendations for the design of compensatory decision aids for use under time pressure. The model is founded on three assumptions: decision-making requires effort, effort is a limited resource, and effort is motivated by vested interes

Experimental investigation of air-cooled turbine blade in turbojet engine VIII : rotor blades with capped leading edges

An air-cooled turbine blade with a capped leading edge was investigated in a modified commercial turbojet engine over a range of engine speed from 4000 to 11,350 rpm. The cooling performance of the caped-leading-edge configuration was superior to all leading-edge cooling modifications previously investigated

New Evidence for Efficient Collisionless Heating of Electrons at the Reverse Shock of a Young Supernova Remnant

Although collisionless shocks are ubiquitous in astrophysics, certain key aspects of them are not well understood. In particular, the process known as collisionless electron heating, whereby electrons are rapidly energized at the shock front, is one of the main open issues in shock physics. Here we present the first clear evidence for efficient collisionless electron heating at the reverse shock of Tycho's supernova remnant (SNR), revealed by Fe-K diagnostics using high-quality X-ray data obtained by the Suzaku satellite. We detect K-beta (3p->1s) fluorescence emission from low-ionization Fe ejecta excited by energetic thermal electrons at the reverse shock front, which peaks at a smaller radius than Fe K-alpha (2p->1s) emission dominated by a relatively highly-ionized component. Comparison with our hydrodynamical simulations implies instantaneous electron heating to a temperature 1000 times higher than expected from Coulomb collisions alone. The unique environment of the reverse shock, which is propagating with a high Mach number into rarefied ejecta with a low magnetic field strength, puts strong constraints on the physical mechanism responsible for this heating, and favors a cross-shock potential created by charge deflection at the shock front. Our sensitive observation also reveals that the reverse shock radius of this SNR is about 10% smaller than the previous measurement using the Fe K-alpha morphology from the Chandra observations. Since strong Fe K-beta fluorescence is expected only from low-ionization plasma where Fe ions still have many 3p electrons, this feature is key to diagnosing the plasma state and distribution of the immediate postshock ejecta in a young SNR.Comment: 7 pages, 9 figures, resubmitted to ApJ with minor changes following the referee repor

Fates of Eroded Soil Organic Carbon: Mississippi Basin Case Study

We have developed a mass balance analysis of organic carbon (OC) across the five major river subsystems of the Mississippi (MS) Basin (an area of 3.2 3 106 km2). This largely agricultural landscape undergoes a bulk soil erosion rate of ;480 t·km22·yr21 (;1500 3 106 t/yr, across the MS Basin), and a soil organic carbon (SOC) erosion rate of ;7 t·km22·yr21 (;22 3 106 t/yr). Erosion translocates upland SOC to alluvial deposits, water impoundments, and the ocean. Soil erosion is generally considered to be a net source of CO2 release to the atmosphere in global budgets. However, our results indicate that SOC erosion and relocation of soil apparently can reduce the net SOC oxidation rate of the original upland SOC while promoting net replacement of eroded SOC in upland soils that were eroded. Soil erosion at the MS Basin scale is, therefore, a net CO2 sink rather than a source.This paper is part of ongoing studies by the coauthors to determine the role of landscape erosion and deposition in material fluxes and biogeochemical cycling. Parts of this work have been supported by internal institutional support at CICESE, Emporia State University, Miami University College of Arts and Science, and the Kansas Geological Survey, and by a Kansas NASA EPSCoR grant awarded to R. W. Buddemeier and R. O. Sleezer.We thank the numerous individuals who contributed technical assistance or conceptual support to these efforts. Three reviewers have provided useful critical comments on versions of this manuscript. Of these, we would like to single out Jon Cole, who thoroughly grasped the big picture of what we were advancing and whose summary comment seems worth quoting: ‘‘The idea that soil erosion is a large net sink of atmospheric CO2 is very interesting, well supported by the arguments and data in this paper, and likely to be a huge controversy. This controversy is a good thing, as Martha Stewart might say.’