Computer Science – Sound
Scientific paper
Nov 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005phdt.........7b&link_type=abstract
Ph.D dissertation, 2005. Section 0051, Part 0606 110 pages; United States -- Colorado: University of Colorado at Boulder; 2005.
Computer Science
Sound
Narrowband, Far-Ultraviolet, Imaging, Shock, Nonradiative
Scientific paper
I have repaired and reflown an existing sounding rocket payload to observe the O VI 1032, 1038 Å emission doublet from a non-radiative shock in the north east section of the Cygnus Loop supernova remnant. I have analyzed the images to determine the total flux emitted by the shock and the distance between the O VI-emitting gas and the shock front in visible light, as well as determining the N (C IV)/ N (O VI) and N (N V)/ N (O VI) column density ratios behind the shock. The purpose of these measurements is to discern between models of the dominant cooling process causing temperature equilibrium of charged particles in the hot shocked gas of the interstellar medium.
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