Wavelength Shifts in the Solar Photospheric Spectrum

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...

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Veröffentlicht in:	Solar physics 2000-09, Vol.196 (1), p.41-50
Hauptverfasser:	Pierce, A Keith, Lopresto, James C
Format:	Artikel
Sprache:	eng
Schlagworte:	Fourier transforms Wavelengths
Online-Zugang:	Volltext
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