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@comment{{Command line: /usr/bin/bib2bib --quiet -c 'not journal:"Discussions"' -c 'not journal:"Polymer Science"' -c year=1975 -c $type="ARTICLE" -oc lmd_EMC31975.txt -ob lmd_EMC31975.bib /home/WWW/LMD/public/Publis_LMDEMC3.link.bib}}
  author = {{Ackerman}, M. and {Fontanella}, J.~C. and {Frimout}, D. and 
	{Girard}, A. and {Louisnard}, N. and {Muller}, C.},
  title = {{Simultaneous measurements of NO and NO2 in the stratosphere}},
  journal = {\planss},
  keywords = {Absorption Spectroscopy, Atmospheric Composition, Infrared Spectroscopy, Nitric Oxide, Nitrogen Dioxide, Stratosphere, Abundance, Air Pollution, Nitrogen Oxides, Solar Radiation},
  year = 1975,
  month = apr,
  volume = 23,
  pages = {651-660},
  abstract = {{NO and NO2 were measured by infrared absorption in the stratosphere,
using the sun as a light source, in the 5.2 and 6.2 micron bands
respectively. These measurements lead to a composite picture of NOx
distribution. The composition reaches a peak at 26 km, where it equals
(4.2 plus or minus 1) times 10 to the ninth power per cu cm. The volume
mixing ratio of NOx varied from 1.3 times 10 to the minus ninth power at
20 km to 1.3 times 10 to the minus eighth power at 34 km.
  doi = {10.1016/0032-0633(75)90105-1},
  adsurl = {https://ui.adsabs.harvard.edu/abs/1975P%26SS...23..651A},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
  author = {{Muller}, C. and {Sauval}, A.~J.},
  title = {{The CO fundamental bands in the solar spectrum}},
  journal = {\aap},
  keywords = {Carbon Monoxide, Molecular Spectra, Solar Spectra, Spectral Bands, Abundance, Balloon Sounding, Infrared Spectra, Photosphere},
  year = 1975,
  month = mar,
  volume = 39,
  pages = {445-451},
  abstract = {{The result of a study of CO lines in the delta v equals 1 bands in the
solar disk spectrum is presented. Recently, the photospheric spectrum
has been recorded using a balloon-borne spectrometer from 40 km
altitude. From a comparison between the observed and synthetic solar
spectra, an agreement is shown using the best available solar and
molecular data. Results are discussed and compared with other
investigations in order to explain an apparent discrepancy between
previous results.
  adsurl = {https://ui.adsabs.harvard.edu/abs/1975A%26A....39..445M},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
  author = {{Muller}, C. and {Lorentz}, B. and {Remy}, M.},
  title = {{Existence of He $^{-}$ ions in a duoplasmatron discharge}},
  journal = {Physics Letters A},
  year = 1975,
  month = jan,
  volume = 51,
  pages = {17-18},
  abstract = {{We point out the presence of He $^{-}$ ions in a duoplasmatron
discharge and detect currents of 10 $^{-15}$ A. The influence of
different parameters on this current is indicated and possible processes
for the formation of He $^{-}$ ions are investigated.
  doi = {10.1016/0375-9601(75)90298-4},
  adsurl = {https://ui.adsabs.harvard.edu/abs/1975PhLA...51...17M},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}