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

Nature volume 244, pages 562–563 (1973)Cite this article

Abstract

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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Author information

Authors and Affiliations

  1. Groupe Infrarouge Spatial, Observatoire de Meudon, 92190—Meudon, France

    J. P. BALUTEAU, E. BUSSOLETTI & N. EPCHTEIN

Authors
  1. J. P. BALUTEAU
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  2. E. BUSSOLETTI
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  3. N. EPCHTEIN
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BALUTEAU, J., BUSSOLETTI, E. & EPCHTEIN, N. Evidence of Features in Atmospheric Spectra at around 8 cm−1 of Probable Solar Origin. Nature 244, 562–563 (1973). https://doi.org/10.1038/244562a0

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