Detection of the H I n=22-21 Rydberg line in emission at the solar submillimetre limb

Details Detection of the H I n=22-21 Rydberg line in emission at the solar submillimetre limb Detection of the H I n=22-21 Rydberg line in emission at the solar submillimetre limb

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...361l..60c&link_type=abstract

Astronomy and Astrophysics, v.361, p.L60-L62 (2000)

Astronomy and Astrophysics

Astrophysics

3

Line: Identification, Sun: Atmosphere, Sun: General, Sun: Infrared

Scientific paper

This letter reports the discovery of excess emission at the position of the H I n=22-21 Rydberg transition in submillimetre solar spectra taken at the extreme solar limb. This emission feature at 22.096+/-0.003 cm-1 shows significant limb brightening, reaching intensities of 11% above the adjacent spectral continuum with line shapes fitted best by Gaussian functions with widths of 0.018+/-0.004 cm-1. This measurement represents the highest-n Rydberg line of H I detected to date in the solar spectrum.

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