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AN EXPERIMENTAL METHOD TO DETERMINE SMALL DIFFERENCES BETWEEN THE POLAR AND EQUATORIAL SOLAR LIMB PROFILESPatz, Douglas Leonard, 1943- January 1975 (has links)
No description available.
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A PRECISE MEASUREMENT OF THE SUN'S VISUAL OBLATENESSClayton, Paul Douglas, 1943- January 1973 (has links)
No description available.
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LONG-PERIOD SOLAR OSCILLATIONS: A SEISMOLOGICAL AND INTERCOMPARATIVE STUDYCaudell, Thomas Preston January 1980 (has links)
This work deals with the subject of global solar oscillations. These oscillations are observed as fluctuations in the diameter of the sun. A diameter is determined by a mathematical solar edge definition at the Santa Catalina Laboratory for Experimental Relativity by Astrometry (SCLERA) instrument. The oscillations have periods ranging from a few minutes to several hours and have amplitudes measured in millionths of a solar radius. These small amplitudes are observable only due to the unique properties of the edge definition. The properties of the observed solar oscillations are determined from the data; their statistical significance and repeatability are then tested. The possibility of using the observed oscillations as a seismic tool for understanding the solar interior and its motions is explored.
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