Oscillations and pulsations

Details Oscillations and pulsations Oscillations and pulsations

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981nassp.450..263l&link_type=abstract

In NASA. Goddard Space Flight Center The Sun as a Star p 263-287 (SEE N81-27008 17-90)

Physics

40

Chromosphere, Electromagnetic Pulses, Photosphere, Solar Oscillations, Wave Propagation, Gas Dynamics, Solar Atmosphere, Solar Physics, Stellar Structure, Sun

Scientific paper

A theory to describe the observed photospheric 5 minute oscillations, chromospheric 3 minute oscillations, and possible motions of the interior with periods ranging from 40 to 160 minutes is discussed. It is similar to the theory of nonradial stellar oscillations developed to describe the low angluar order modes (one or two wavelengths around a circumference); however, the solar oscillations have thousands of wavelengths around a circumference. The properties of waves in stars, their restoring forces, periods and wavelengths, and their propagation and motions are discussed.

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