Sensitivity of inferred subphotospheric velocity field to mode selection, analysis technique and noise

Details Sensitivity of inferred subphotospheric velocity field to mode selection, analysis technique and noise Sensitivity of inferred subphotospheric velocity field to mode selection, analysis technique and noise

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sses.nasa...95h&link_type=abstract

In JPL Solar Seismology from Space. p 95-111 (SEE N85-25060 14-92)

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3

Applications Of Mathematics, Helioseismology, Photosphere, Solar Oscillations, Velocity Distribution, Solar Activity, Solar Rotation, Stellar Structure, Sun

Scientific paper

The horizontal velocity immediately below the photosphere can be inferred from observations of high-degree solar oscillations by an optimal-averaging inversion technique. The authors investigate the sensitivity of the results to various details of both the inversion and the determination of the frequencies. The results are shown to be quite stable to the choice of most parameters, suggesting that this procedure produces reliable estimates of the subsurface velocity.

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