Simulating photospheric Doppler velocity fields

Details Simulating photospheric Doppler velocity fields Simulating photospheric Doppler velocity fields

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..117..329h&link_type=abstract

(Solar Cycle Workshop, Meeting, 2nd, Lake Tahoe, CA, May 1987) Solar Physics (ISSN 0038-0938), vol. 117, no. 2, 1988, p. 329-341

Physics

12

Computerized Simulation, Laser Doppler Velocimeters, Photosphere, Solar Rotation, Atmospheric Scattering, Solar Granulation, Solar Observatories, Solar Oscillations, Velocity Distribution

Scientific paper

A method is described for constructing artificial data that realistically simulate photospheric velocity fields. The velocity fields include rotation, differential rotation, meridional circulation, giant cell convection, supergranulation, convective limb shift, p-mode oscillations, and observer motion. Data constructed by this method can be used for testing algorithms designed to extract and analyze these velocity fields in real Doppler velocity data.

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