A more accurate wavelength for the red coronal line

Details A more accurate wavelength for the red coronal line A more accurate wavelength for the red coronal line

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..559t&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, Dec. 1977, p. 559-561. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Line Spectra, Solar Corona, Solar Spectra, Distribution Functions, Doppler Effect, Red Shift, Statistical Analysis, Wavelengths

Scientific paper

An improved wavelength value is computed for the red coronal line on the basis of two data sets consisting, respectively, of 1500 and 5000 Doppler shifts observed at the east and west limbs of the sun. The result obtained from the larger sample is 6374.5492 + or - 0.0011 A. It is noted that the statistical accuracy is no worse than the instrument accuracy of 0.001 A.

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