Magnetically induced spectral line redshifts full disk measurements

Details Magnetically induced spectral line redshifts full disk measurements Magnetically induced spectral line redshifts full disk measurements

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..325u&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 325-332 (SEE N89-25819 19-92)

Physics

1

Magnetic Effects, Red Shift, Solar Spectra, Sun, Calibrating, Helioseismology, Spectrum Analysis

Scientific paper

A method which allows the calibration of the magnetically induced velocities and permits an improvement of the information from various planned solar oscillation experiments is presented. Based on the differential sensitivity to the magnetic effects of various spectral lines, a correction function giving the Doppler shift in each line as a function of the difference between shifts of the lines is derived. For 5250 A, the correction to be added to the observed velocity is -0.9 + or - 0.1 (V = 5237 to 5250).

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