Computer Science – Sound
Scientific paper
Oct 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979lock.reptr....l&link_type=abstract
Final Report Lockheed Missiles and Space Co., Palo Alto, CA.
Computer Science
Sound
Chromosphere, Oso-8, Photosphere, Solar Spectra, Stellar Atmospheres, Ultraviolet Astronomy, Internal Waves, Line Spectra, Lyman Alpha Radiation, Sound Waves, Spaceborne Astronomy, Sun
Scientific paper
Data obtained by the Laboratoire de Physique Stellaire et Planetaire's ultraviolet spectrometer onboard the OSO-8 spacecraft were analyzed in an effort to dynamically model the solar chromosphere as an aid in enhancing knowledge of the dynamical processes themselves and of spectral line formation in the dynamic chromosphere. Repeated spectral scans of strong, optically thick resonance lines formed in the solar chromosphere were examined for indications of oscillatory velocities and intensities among other indications of velocity which were studied, the blue peak is reasonably well defined, and the position of a parabolic filter fitted by the least squares method was used to define it. Observed chromospheric oscillation periods are discussed as well as the variations in altitude of the emitting region which result primarily from the motion up and down during the oscillation.
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