Computer Science – Sound
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sses.nasa....7t&link_type=abstract
In JPL Solar Seismology from Space. p 7-39 (SEE N85-25060 14-92)
Computer Science
Sound
1
Helioseismology, Solar Activity, Solar Interior, Solar Oscillations, Stellar Structure, Doppler Effect, Gravitational Waves, Mathematical Models, Photosphere, Solar Rotation, Sound Waves, Space Observations (From Earth), Sun
Scientific paper
The physical nature of solar oscillations is reviewed. The nomenclature of the subject and the techniques used to interpret the oscillations are discussed. Many of the acoustic and gravity waves that can be observed in the atmosphere of the Sun are actually resonant or standing modes of the interior; precise measurements of the frequencies of such modes allow deductions of the internal structure and dynamics of this star. The scientific objectives of such studies of solar seismic disturbances, or of solar seismology, will be outlined. The reasons for why it would be very beneficial to carry out further observations of solar oscillations both from ground-based networks and from space will be discussed.
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