The use of molecular iodine absorption lines as wavelength references for solar Doppler shift measurements

Details The use of molecular iodine absorption lines as wavelength references for solar Doppler shift measurements The use of molecular iodine absorption lines as wavelength references for solar Doppler shift measurements

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...134..134k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 134, no. 1, May 1984, p. 134-138. Research supported by the Deutsche Forschung

Astronomy and Astrophysics

Astrophysics

14

Doppler Effect, Frequency Shift, Iodine, Solar Spectra, Wavelengths, Absorption Spectra, Line Spectra

Scientific paper

Molecular iodine absorption lines are used as wavelength references for solar Doppler shift measurements near 5576 Å and 5612 Å. The possible shifts of these wavelength references caused by weak lines in the solar continuum used as the light source, are investigated by measurements and numerical model calculations. Within the solar spectrum from 5000 Å to 6000 Å optimum windows are given for the use of iodine reference lines.

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