A comparative study of imtermediate P-mode pressure-wave propagation in the sun /
30 percent of its radius. This corresponds to the
| Main Author: | |
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| Format: | Thesis eBook |
| Language: | English |
| Published: |
[Place of publication not identified] :
[publisher not identified] ;
1996.
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| Subjects: | |
| Online Access: | Link to OAKTrust copy |
| Summary: | 30 percent of its radius. This corresponds to the and magnetic-field interacttons math the plasma are approxffnate depth of the lower boundary of the sun's between 20 and 100 are used to image the sun's s in the outer By analyzing the observed frequencies of solar P-mode convection zone. down to the core. 'Me intermediate P-modes with I-values frequencies of these oscillations is obtained by observing gravitating ideal gas. The effects of convection, rotation in this frequency range allows for irnvng of the sun's s c knowledge about the density, rate of rotation, temperature, neglected. The observed cies of oscillation lie 'in the pressure and composition of the sun in its interior. The pressure waves, it has been possible to obtain detailed range of approximately 16OO-4800 []Hz.. P-waves oscillating the Doppler shifting of the Fraunhofer absorption lines in the sun's optical spectrum. The sun is modeled as a self- |
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| Item Description: | "Major subject: Geophysics". Vita. |
| Physical Description: | x, 69 leaves : illustrations ; 28 cm. Also available online. Issued also on microfiche from Lange Micrographics. |
| Bibliography: | Includes bibliographical references. |