lmd_EMC31976.bib

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@article{1976GeoRL...3...81A,
  author = {{Ackerman}, M. and {Frimout}, D. and {Girard}, A. and {Gottignies}, M. and 
	{Muller}, C.},
  title = {{Stratospheric HCl from infrared spectra}},
  journal = {\grl},
  keywords = {Aeronomy: Composition (atomic or molecular), Meteorology: Air quality, Meteorology: Chemical composition and chemical interactions},
  year = 1976,
  month = feb,
  volume = 3,
  pages = {81-83},
  abstract = {{HCl has been observed in the stratosphere from balloon borne
spectroscopic measurements of a portion of the fundamental band in the 3
microns wavelength region. The observation of absorption lines using the
sun as a source at solar zenith angles larger than 90{\deg} indicates an
HCl volume mixing ratio equal to (3.8 {\plusmn} 1.5) {\times}
10$^{-10}$ at 20 km increasing with altitude at least up to
30 km where the value is (1.4 {\plusmn} 0.6) {\times}
10$^{-9}$. The total zenith amount above 21 km is found to
be (10{\plusmn} 3.5) {\times} 10$^{-14}$ cm$^{-2}$
in agreement with previous observations performed up to this altitude. A
maximum number density equal to (7.2 {\plusmn} 3) {\times} 10$^{8}$
cm$^{-3}$ is observed at 24 {\plusmn} 2 km altitude.
}},
  doi = {10.1029/GL003i002p00081},
  adsurl = {https://ui.adsabs.harvard.edu/abs/1976GeoRL...3...81A},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}