Identifications of solar lines out to 8 microns, based on spectra obtained by balloon

Details Identifications of solar lines out to 8 microns, based on spectra obtained by balloon Identifications of solar lines out to 8 microns, based on spectra obtained by balloon

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....56..315b&link_type=abstract

Astronomy and Astrophysics, vol. 56, no. 1-2, Apr. 1977, p. 315-317. Research supported by the Fonds de la Recherche Fondamenta

Computer Science

Sound

1

Atomic Spectra, Balloon Sounding, Infrared Spectra, Line Spectra, Solar Spectra, Balloon-Borne Instruments, High Altitude Balloons, Photosphere, Spectral Resolution

Scientific paper

The identification of 32 atomic solar lines, obtained from
high-resolution infrared spectra (at wavelengths of 3.3 to 8.0 microns)
recorded during stratospheric balloon flights, is presented.
Photospheric atomic lines have been identified with certainty out to 8
microns

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