13,323 research outputs found

    The Second-Person Perspective in the Preface of Nicholas of Cusa’s De Visione Dei

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    In De visione Dei’s preface, a multidimensional, embodied experience of the second-person perspective becomes the medium by which Nicholas of Cusa’s audience, the benedictine brothers of Tegernsee, receive answers to questions regarding whether and in what sense mystical theology’s divine term is an object of contemplation, and whether union with God is a matter of knowledge or love. The experience of joint attention that is described in this text is enigmatic, dynamic, integrative, and transformative. As such, it instantiates the coincidentia oppositorum and docta ignorantia which, for Cusa, alone can give rise to a vision of the infinite

    DELIVERING SAFE FOOD TO CONSUMERS

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    Food Consumption/Nutrition/Food Safety,

    A SURVEY OF LARGE SPACE CHAMBERS

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    Survey of large space chambers - vacuum chambers to simulate space environmen

    Constraints on fault and lithosphere rheology from the coseismic slip and postseismic afterslip of the 2006 M_w 7.0 Mozambique earthquake

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    The 2006 M_w 7.0 Mozambique (Machaze) normal-faulting earthquake ruptured an unusually steeply dipping fault plane (~75°). The amount of slip in the earthquake decreased from depths of ~10 km toward the surface, and this shallow slip deficit was at least partly recovered by postseismic afterslip on the shallow part of the fault plane. An adjacent normal fault segment slipped postseismically (and possibly also co-seismically) at shallow depths with a large strike-slip component, in response to the stresses generated by slip on the main earthquake fault plane. Our observations suggest that the fault zone behaves in a stick-slip manner in the crystalline basement, and that where it cuts the sedimentary layer the coseismic rupture was partially arrested and there was significant postseismic creep. We discuss the effects of such behavior on the large-scale tectonics of continental regions, and on the assessment of seismic hazard on similar fault systems. The steep dip of the fault suggests the re-activation of a preexisting structure with a coefficient of friction at least ~25–45% lower than that on optimally oriented planes, and analysis of the deformation following an aftershock indicates that the value of the parameter ‘a’ that describes the rate-dependence of fault friction lies in the range 1 × 10^(−3)–2 × 10^(−2). The lack of long-wavelength postseismic relaxation suggests viscosities in the ductile lithosphere of greater than ~2 × 10^(19) Pa s, and an examination of the tectonic geomorphology in the region identifies ways in which similar fault systems can be identified before they rupture in future earthquakes

    Transport of Mars atmospheric water into high northern latitudes during a polar warming

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    Several numerical experiments were conducted with a simplified tracer transport model in order to attempt to examine the poleward transport of Mars atmospheric water during a polar warming like that which occurred during the winter solstice dust storm of 1977. The flow for the transport experiments was taken from numerical simulations with a nonlinear beta-plane dynamical model. Previous studies with this model have demonstrated that a polar warming having essential characteristics like those observed during the 1977 dust storm can be produced by a planetary wave mechanism analogous to that responsible for terrestrial sudden stratospheric warmings. Several numerical experiments intended to simulate water transport in the absence of any condensation were carried out. These experiments indicate that the flow during a polar warming can transport very substantial amounts of water to high northern latitudes, given that the water does not condense and fall out before reaching the polar region

    Numerical simulations of dust transport into northern high latitudes during a Martian polar warming

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    The formation and evolution of the polar laminated terrain depends on rates of dust transport to the polar caps. A simplified dynamical model is shown similar to models used to simulate terrestrial stratospheric polar warmings could simulate certain observed features of the circulation during Martian global dust storms. Model simulations of dust transport showed that substantial quantities of dust, enough to produce optical depths of approx. 1, could reach the pole during these storms
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