3,022 research outputs found

    The Call of Duty and Beyond: Problems Concerning Justification and Virtue in the Ethical Models of Epistemology

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    Internalist considerations are crucial to a good theory of belief formation—epistemic or ethical. To get to this conclusion, the author first shows the insufficiency of a strong externalist account of true belief; he critique’s Plantinga’s reliabilism by way of demonstration. Plantinga’s idea of epistemic warrant shares a maximum ideal with utilitarianism (the desire for the most true beliefs), but the good intentions of the theory are undermined by 1) the author’s car counter-example that illustrates the relevance of internal circumstances, and 2) a realization that Plantinga pays no mind to volition variance. Next, the author analyzes Linda Trinkaus Zagzebski’s virtue ethics and notes its own form of reliabilism but promising internalist account of justification. Despite the fact that both theorists can be used improperly to reward vicious means to ends, such as guessing, Zagzebski’s virtue ethics improves the reliability of Plantinga’s epistemology

    The “missing” politics of whiteness and rightful presence in the settler colonial city

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    This is the author accepted manuscript. The final version is available from Sage publications via the DOI in this record.This paper engages the global nexus of colonization, racialization, and urbanization through the settler colonial city of Kelowna, British Columbia (BC), Canada. Kelowna is known for its recent, rapid urbanization and for its ongoing, disproportionate ‘whiteness,’ understood as a complex political geography that enacts boundaries of inclusion and exclusion. The white urban identity of Kelowna defines Indigenous and migrant communities as ‘missing’ or ‘out-of-place,’ yet these configurations of ‘missing’ are politically contested. This paper examines how differential processes of racialization and urbanization establish the whiteness of this settler-colonial city, drawing attention to ways that ‘missing’ communities remake relations of ‘rightful presence’ in the city, against dominant racialized, colonial, and urban narratives of their absence and processes of their displacement. Finally, this paper considers how a politics of ‘rightful presence’ needs to be reconfigured in the settler-colonial city, which itself has no rightful presence on unceded Indigenous land

    IRAS asteroid families

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    The Infrared Astronomical Satellite (IRAS) sampled the entire asteroid population at wavelengths from 12 to 100 microns during its 1983 all sky survey. The IRAS Minor Planet Survey (IMPS) includes updated results for more recently numbered as well as other additional asteroids with reliable orbital elements. Albedos and diameters were derived from the observed thermal emission and assumed absolute visual magnitudes and then entered into the IMPS database at the Infrared Processing and Analysis Center (IPAC) for members of the Themis, Eos, Koronis and Maria asteroid families and compared with their visual colors. The IMPS results for the small (down to about 20 km) asteroids within these major families confirm trends previously noted for their larger members. Each of these dynamical families which are defined by their similar proper elements appears to have homogeneous physical properties

    Retrieval of Dry Snow Parameters from Radiometric Data Using a Dense Medium Model and Genetic Algorithms

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    In this paper, GA-based techniques are used to invert the equations of an electromagnetic model based on Dense Medium Radiative Transfer Theory (DMRT) under the Quasi Crystalline Approximation with Coherent Potential to retrieve snow depth, mean grain size and fractional volume from microwave brightness temperatures. The technique is initially tested on both noisy and not-noisy simulated data. During this phase, different configurations of genetic algorithm parameters are considered to quantify how their change can affect the algorithm performance. A configuration of GA parameters is then selected and the algorithm is applied to experimental data acquired during the NASA Cold Land Process Experiment. Snow parameters retrieved with the GA-DMRT technique are then compared with snow parameters measured on field

    A ring as a model of the main belt in planetary ephemerides

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    We assess the ability of a solid ring to model a global perturbation induced by several thousands of main-belt asteroids. The ring is first studied in an analytical framework that provides an estimate of all the ring's parameters excepting mass. In the second part, numerically estimated perturbations on the Earth-Mars, Earth-Venus, and Earth-Mercury distances induced by various subsets of the main-belt population are compared with perturbations induced by a ring. To account for large uncertainties in the asteroid masses, we obtain results from Monte Carlo experiments based on asteroid masses randomly generated according to available data and the statistical asteroid model. The radius of the ring is analytically estimated at 2.8 AU. A systematic comparison of the ring with subsets of the main belt shows that, after removing the 300 most perturbing asteroids, the total main-belt perturbation of the Earth-Mars distance reaches on average 246 m on the 1969-2010 time interval. A ring with appropriate mass is able to reduce this effect to 38 m. We show that, by removing from the main belt ~240 asteroids that are not necessarily the most perturbing ones, the corresponding total perturbation reaches on average 472 m, but the ring is able to reduce it down to a few meters, thus accounting for more than 99% of the total effect.Comment: 18 pages, accepted in A&
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