Computer Science
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sses.nasa..207c&link_type=abstract
In JPL Solar Seismology from Space. p 207-217 (SEE N85-25060 14-92)
Computer Science
1
Eigenvectors, Solar Activity, Solar Limb, Solar Oscillations, Spatial Resolution, Temporal Resolution, Fourier Transformation, Perturbation, Solar Atmosphere, Thermodynamic Properties
Scientific paper
Solar oscillations are manifested in the solar atmosphere as spatial and temporal perturbations in the local thermodynamical and mechanical properties. When measuring the solar radius/diameter, these perturbations enter the observation through changes in the radiative source function and opacity at the extreme limb. When compared to the disk center, the observable portion of these perturbations is changed in spatial character by projection effects and oblique optical depth geometry. The time varying solar radius signal at SCLERA (Santa Catalina Laboratory for Experimental Relativity) is produced by an edge definition sensitive to the resultant changes in the spatial shape of the limb intensity profile. An attempt is made to further determine the shape and properties of the limb signals which display global solar oscillations.
Bos Randall J.
Caudell Thomas P.
Hill Adrian H.
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