Observations of individual solar eigenmodes: Their properties and implications

Details Observations of individual solar eigenmodes: Their properties and implications Observations of individual solar eigenmodes: Their properties and implications

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phdt.........7b&link_type=abstract

Ph.D. Thesis Arizona Univ., Phoenix.

Physics

8

Harmonic Analysis, Solar Limb, Solar Oscillations, Spatial Resolution, Atmospheric Effects, Data Acquisition, Eigenvalues, Fourier Transformation, Signal Processing, Solar Rotation

Scientific paper

Data taken in 1979 using a modification of the solar detector at SCLERA (Santa Catalina Laboratory for Experimental Relativity) designed to enhance spatial properties of the previously observed solar oscillations was analyzed. Unlike previous solar observations taken at SCLERA, where the data consisted of single solar diameter measurements, the 1979 data consisted of six recorded limb profiles. This has important ramifications for the amount of signal present in the data which was generated by the terrestrial atmosphere, for the origin of the observed solar oscillations in fluctuations of the solar limb darkening function, and, most importantly, for the spatial symmetry properties of the observed solar eigenfunctions.

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