Wavelength Shifts in the Solar Photospheric Spectrum

Details Wavelength Shifts in the Solar Photospheric Spectrum Wavelength Shifts in the Solar Photospheric Spectrum

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..196...41p&link_type=abstract

Solar Physics, v. 196, Issue 1, p. 41-50 (2000).

Physics

1

Scientific paper

Wavelength shifts converted to velocities between solar lines observed at disc center and laboratory wavelengths of Fei, Feii, Tii, Nii, and Fei lines in the near infrared are plotted as a function of the logarithm of their solar equivalent width in milliångstroms. The need for wavelengths based on the wavelength standards is stressed. A comparison of photographic Fei solar wavelength is shown to agree, on the average, with Fourier Transform Spectrometer solar wavelengths within less than 0.5 milliångstroms. Using Balthasar's limb effect tables we convert the disc center velocities to limb velocities and find, though the scatter is large, that there is little evidence for a super-gravitational red shift.

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