Solar rotation measurements at Mount Wilson. I - Analysis and instrumental effects

Details Solar rotation measurements at Mount Wilson. I - Analysis and instrumental effects Solar rotation measurements at Mount Wilson. I - Analysis and instrumental effects

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...66..167h&link_type=abstract

Solar Physics, vol. 66, May 1980, p. 167-185.

Physics

41

Magnetic Measurement, Red Shift, Solar Magnetic Field, Solar Rotation, Velocity Distribution, Doppler Effect, Least Squares Method, Nonlinearity, Solar Limb

Scientific paper

We examine the background velocity fields of the sun as observed at Mount Wilson. The method of velocity reduction of the full-disk Mount Wilson data is outlined. We describe a number of tests that have been carried out in order to find an instrumental origin for short-term rotation variations and a large-scale background line-shift - the ears. No instrumental cause can be found for this ear effect, although such a cause cannot yet be ruled out.

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