Jet quenching parameters in strongly coupled nonconformal gauge theories This suggests that observed beams undergo earlier processing, if they are present at all. Finally, we present synthetic emission images of HÎ± and and note an excess of emission along the jet length as compared to observations. Our results indicate that a large velocity dispersion leads to a clump-clump collision-dominated flow which disrupts the jet beam. The goodness of fits, while poor in all simulations, are best when clump-clump collisions are minimal. We here extend the results presented in Yirak et al., including how analysis of individual observations may lead to spurious sinusoidal variation whose parameters vary widely over time, owing chiefly to interactions between clumps. By varying clumps' size, density, position, and velocity, we cover a range of parameter space motivated by observations of objects such as the Herbig-Haro object HH 34. We investigate the role discrete clumps embedded in an astrophysical jet play on the jet's morphology and line emission characteristics. Yirak, Kristopher Schroeder, Ed Frank, Adam Cunningham, Andrew J. THE EVOLUTION OF HETERGENEOUS 'CLUMPY JETS': A PARAMETER STUDY The appendix presents the parameters of the DEMO and NET under the topic headings: power, geometry, plasma, toroidal and poloidal magnetic field coils, first wall engineering, divertor physics, divertor engineering, and blanket. The latter study examines whether the technologies and design principles proposed for NET can be directly extrapolated to a demonstration (DEMO) reactor. The paper is an appendix to a study of the reactor relevance of the NET design concept. International Nuclear Information System (INIS)

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