Some Solar Lines in the Infra-Red Spectrum observed from a High-Flying Aircraft

Details Some Solar Lines in the Infra-Red Spectrum observed from a High-Flying Aircraft Some Solar Lines in the Infra-Red Spectrum observed from a High-Flying Aircraft

Mar 1961

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1961natur.189..908h&link_type=abstract

Nature, Volume 189, Issue 4768, pp. 908-909 (1961).

Physics

Scientific paper

IN a previous communication1, it was pointed out that strong absorption by atmospheric constituents obscures large parts of the infra-red spectrum from ground-level observation. However, by working at high altitudes and by using a high-resolution spectrometer, it is possible to observe additional features due to absorption in the solar atmosphere. Among these are two absorption lines due to the electronic transitions in solar hydrogen 3-4 and 4-8, which occur in the great water-vapour band at 1.9µ.

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