Physics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.1011c&link_type=abstract
American Astronomical Society Meeting 205, #10.11; Bulletin of the American Astronomical Society, Vol. 36, p.1351
Physics
Scientific paper
Application of a new physics-based background subtraction method has allowed for investigation of the physical properties of coronal loops with unprecedented accuracy. We determine the temperature, emission measure, and pressure along multiple EUV coronal loops as a function of time and space, as well as their cross-section. With these measures of physical observables we have calculated the rate of change of pressure for the loops.
Cirtain Jonathan W.
Martens Petrus C. H.
Scott John T.
Winter Henry D.
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