The basic equations for scanning heliometer measurement of solar diameters

Details The basic equations for scanning heliometer measurement of solar diameters The basic equations for scanning heliometer measurement of solar diameters

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...96..213r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 96, April 1985, p. 213-217.

Physics

4

Astrometry, Heliometers, Solar Diameter, Solar Oblateness, Solar Oscillations, Data Processing, Helioseismology, Scanners, Secular Variations

Scientific paper

After presenting the basic equations for measurement of solar diameters by means of a scanning heliometer, attention is given to the processing of the rough data for the cases of oblateness evaluation, medium term oscillation detection, and the investigation of secular diameter changes. Corrective terms are applied for solar oblateness, for the shift of the inflection point of the profile toward the center of the disk, and for image motion which transports each limb by a random amount.

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