Evidence of Features in Atmospheric Spectra at around 8 cm-1 of Probable Solar Origin

Details Evidence of Features in Atmospheric Spectra at around 8 cm-1 of Probable Solar Origin Evidence of Features in Atmospheric Spectra at around 8 cm-1 of Probable Solar Origin

Aug 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973natur.244..562b&link_type=abstract

Nature, Volume 244, Issue 5418, pp. 562-563 (1973).

Computer Science

4

Scientific paper

OUR studes of emission spectra of the stratosphere in the frequency
range 30 to 200 cm-1 from a Caravelle1,2 have
revealed lines due to the principal atmospheric components
H2O, O2 and O3.

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