Accession Number : AD0725870
Title : A Study of the Five-Minute Oscillations, Supergranulation, and Related Phenomena in the Solar Atmosphere.
Descriptive Note : Technical rept.,
Corporate Author : CALIFORNIA UNIV BERKELEY DEPT OF PHYSICS
Personal Author(s) : Tanenbaum,Andrew S.
Report Date : 20 MAY 1971
Pagination or Media Count : 146
Abstract : In the early 1960's two new types of motion in the sun's atmosphere were discovered: the 5-minute oscillations and the supergranulation. The 5-minute oscillations consist of a predominantly vertical hydrodynamic wave motion in the photosphere and chromosphere with amplitudes around 500 meters/sec. The supergranulation consists of a series of convective cells, 30,000 km in diameter, in which material rises at the center, flows horizontally outward, and falls at the boundaries. The horizontal motion in the supergranulation was clearly observed, but its vertical motion was observed only marginally at best. The observations that form the basis of this thesis were made at the Mt. Wilson Observatory 150-foot solar telescope. The observing equipment is described in detail, including the optics, guiding and scanning system, spectrograph, magnetograph, electronics, and data system. The observing procedure used in these observations is carefully described, as is the method of calibrating the doppler, Zeeman, and intensity signals. The initial data reduction is also discussed. Various measurements of the size and lifetime of the 5-minute oscillations are reported. (Author)
Descriptors : (*SOLAR ATMOSPHERE, ATMOSPHERIC MOTION), CHROMOSPHERE, SOLAR DISTURBANCES, EQUATIONS OF MOTION, HYDRODYNAMICS, ZEEMAN EFFECT, DOPPLER EFFECT, MAGNETIC FIELDS, MAGNETOMETERS, ELECTRONIC EQUIPMENT, DATA PROCESSING, THESES
Subject Categories : Astrophysics
Distribution Statement : APPROVED FOR PUBLIC RELEASE