Interpretation and Social Explanation

In this article I focus on those aspects of Keith Dowding’s book that are most concerned with interpretive approaches to the study of politics. I argue that, in ways not adequately captured by Dowding’s descriptions, the historical study of political concepts tells us something about their historical political effects and for this reason has a distinct value for how we think about and study politics. Furthermore, I argue, concepts of and about politics, including the concepts of political science, cannot be fully separated from the political contexts of which they are a part. Concepts which function as generalisable explanations at one point in time can shape the thinking and behaviour of political actors and thus be very particular causes. A philosophy or method of political science unaware of or inattentive to this dimension of politics and political science is incomplete

Nonmigrating semidiurnal tide over the Arctic determined from TIMED Doppler Interferometer wind observations

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94847/1/jgrd15899.pd

Epistemic freedom and education

First of all, I define the concept of epistemic freedom in the light of the changing nature of educational practice that prioritise over-prescriptive conceptions of learning. I defend the ‘reality’ of this freedom against possible determinist-related criticisms. I do this by stressing the concept of agency as characterised by ‘becoming’. I also discuss briefly some of the technical literature on the subject. I then move on to discuss Gramsci’s concept of hegemony and Foucault’s idea of ‘productive power’: I argue for the need of a counter-narrative of freedom that takes the form of a genealogy. Finally I discuss in more detail the nature of epistemic freedom and briefly discuss the ethical implications of the concept

Evaluation of an Electrostatic Dust Removal System with Potential Application in Next-Step Fusion Devices

The ability to manage inventories of carbon, tritium, and high-Z elements in fusion plasmas depends on means for effective dust removal. A dust conveyor, based on a moving electrostatic potential well, was tested with particles of tungsten, carbon, glass and sand. A digital microscope imaged a representative portion of the conveyor, and dust particle size and volume distributions were derived before and after operation. About 10 cu mm volume of carbon and tungsten particles were moved in under 5 seconds. The highest driving amplitude tested of 3 kV was the most effective. The optimal driving frequency was 210 Hz (maximum tested) for tungsten particles, decreasing to below 60 Hz for the larger sand particles. Measurements of particle size and volume distributions after 10 and 100 cycles show the breaking apart of agglomerated carbon, and the change in particle distribution over short timescales 1 s)

On the source, site and modes of domination

This article seeks to examine how domination manifests in social relationships and institutions. It does this by examining two debates in republican literature. The first of which is whether domination requires institutionalisation? This addresses the source of domination. The second debate is on the nature of arbitrary power. This raises questions about the site of domination. It will be argued that the source of domination can be personally or socially constituted and that the site can be interactional or systemic. This yields four modes of domination that can be used to examine social institutions and relationships

Circumstellar Na I and Ca II lines in type IIP supernovae and SN 1998S

We study a possibility of detection of circumstellar absorption lines of Na I D$_{1,2}$ and Ca II H,K in spectra of type IIP supernovae at the photospheric epoch. The modelling shows that the circumstellar lines of Na I doublet will not be seen in type IIP supernovae for moderate wind density, e.g., characteristic of SN 1999em, whereas rather pronounced Ca II lines with P Cygni profile should be detectable. A similar model is used to describe Na I and Ca II circumstellar lines seen in SN 1998S, type IIL with a dense wind. We show that line intensities in this supernova are reproduced, if one assumes an ultraviolet excess, which is caused primarily by the comptonization of supernova radiation in the shock wave.Comment: To be published in Astronomy Letter

TIMED Doppler Interferometer on the Thermosphere Ionosphere Mesosphere Energetics and Dynamics satellite: Data product overview

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94699/1/jgra18252.pd