Spatial filtering of global oscillations of the sun with a low degree L

Details Spatial filtering of global oscillations of the sun with a low degree L Spatial filtering of global oscillations of the sun with a low degree L

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...11b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, July-Aug. 1986, p. 11-20. In Russian.

Statistics

Computation

Solar Oscillations, Spatial Filtering, Telescopes, Amplitudes, Sensitivity, Signal Analysis, Tables (Data), Vibration Mode

Scientific paper

Sensitivity functions (spatial response) functions to global solar oscillations for degrees l = 0-21 are computed for spatial filters of the Crimean, Stanford, and Nice telescopes. Computational results are given for both radial and horizontal oscillation components, and the computation procedure is briefly described. The amplitudes of 160-min oscillations were observed with the above-mentioned three telescopes, and a value of l = 2 is found to be likely.

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