2000
DOI: 10.1364/ao.39.000386
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SALOMON: a new, light balloonborne UV–visible spectrometer for nighttime observations of stratospheric trace-gas species

Abstract: A new, light balloonborne UV-visible spectrometer, called SALOMON, is designed to perform nighttime measurements of stratospheric trace-gas species by using the Moon as a light source. The first flight, performed on 31 October 1998 at mid-latitude with a float altitude of 26.7 km, allowed the performance of the pointing system to be checked and vertical profiles of ozone, NO(2), NO(3), and possibly OBrO to be obtained. First the instrument and then the performance of the pointing system and the detector are de… Show more

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Cited by 33 publications
(34 citation statements)
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References 15 publications
(24 reference statements)
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“…The Fraunhoffer lines of the moon spectra do not allow the direct estimation of the NO3 contribution in the reference spectrum. In this case, large negative values appear during the retrieval: the most negative value obtained provides an estimate of this contribution, or at least its lower limit [Renard et al, 2000]. Here the correction is equal to 4 1014 cm -2, which corresponds to 50% of the maximum of the slant column densities profile.…”
Section: No3 Retrievalmentioning
confidence: 87%
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“…The Fraunhoffer lines of the moon spectra do not allow the direct estimation of the NO3 contribution in the reference spectrum. In this case, large negative values appear during the retrieval: the most negative value obtained provides an estimate of this contribution, or at least its lower limit [Renard et al, 2000]. Here the correction is equal to 4 1014 cm -2, which corresponds to 50% of the maximum of the slant column densities profile.…”
Section: No3 Retrievalmentioning
confidence: 87%
“…The description of the NO3 retrieval from balloonborne measurements is given by Renard et al [1996Renard et al [ , 1999aRenard et al [ , 2000. Nevertheless, some specific points will be discussed here.…”
Section: No3 Retrievalmentioning
confidence: 99%
“…Vertical concentration profiles have been derived using an a posteriori least-squares inversion technique (Rodgers et al, 2000), taking into account the fitting error and the uncertainties of the cross sections. Note that the data reduction method used in this study is described by Renard et al (2000) and Berthet et al (2002). For the flight presented in this study we have added an HR4000 UV spectrometer from Ocean Optics to detect BrO absorption lines in the 346-360 nm range as done for the DOAS instrument.…”
Section: A4 the Salomon Remote-sensing Uv-visible Spectrometermentioning
confidence: 99%
“…On 25 August 2009, we flew a successor of the former SALOMON instrument, which was described by Renard et al (2000). The new version of the instrument is able to either use the Moon or the Sun as light source.…”
Section: Balloon-borne and Ground-based Observationsmentioning
confidence: 99%