Aircraft Observations of the Spectra of Jupiter Between 16 and 60 Microns: A Determination of the Helium to Hydrogen Ratio and the Vertical Temperature Structure

Details Aircraft Observations of the Spectra of Jupiter Between 16 and 60 Microns: A Determination of the Helium to Hydrogen Ratio and the Vertical Temperature Structure Aircraft Observations of the Spectra of Jupiter Between 16 and 60 Microns: A Determination of the Helium to Hydrogen Ratio and the Vertical Temperature Structure

Jun 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974baas....6..377h&link_type=gif

Bulletin of the American Astronomical Society, Vol. 6, p.377

Astronomy and Astrophysics

Astronomy

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