2012
DOI: 10.1175/bams-d-11-00135.1
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OSIRIS: A Decade of Scattered Light

Abstract: It is the trace composition of the atmosphere that governs the chemistry of the lower and middle atmosphere and to a large extent the climate of our planet. Accurately determining the abundance of species such as ozone (~1 ppm), nitrogen dioxide (~1 ppb), or bromine monoxide (~1 ppt) presents a large challenge. Further determining how they vary in space and time on a global scale is even more daunting. A global view of the atmospheric trace gas and aerosol composition can only be achieved from space via remote… Show more

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Cited by 38 publications
(35 citation statements)
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“…The instrument performed occultations of selected stars by means of four spectrometers. We use aerosol extinction profiles at 550 nm retrieved by the Aer-GOM algorithm, which was developed using an improved aerosol parameterization (McLinden et al, 2012). The primary instrument is an optical spectrograph (OS) operating in the 284-810 nm range and providing between 100 and 400 vertical profiles per day depending on the time of year.…”
Section: Satellite Aerosol Soundersmentioning
confidence: 99%
“…The instrument performed occultations of selected stars by means of four spectrometers. We use aerosol extinction profiles at 550 nm retrieved by the Aer-GOM algorithm, which was developed using an improved aerosol parameterization (McLinden et al, 2012). The primary instrument is an optical spectrograph (OS) operating in the 284-810 nm range and providing between 100 and 400 vertical profiles per day depending on the time of year.…”
Section: Satellite Aerosol Soundersmentioning
confidence: 99%
“…The OSIRIS instrument began standard stratospheric limb scattered sunlight measurements in early 2002, shortly after launch on the Odin satellite in 2001 (Llewellyn et al, 2004;Murtagh et al, 2002;McLinden et al, 2012) and remains fully operational at the present time. The spectra, which cover the 280-800 nm wavelength range, are used in combination with a spherical radiative transfer model that accounts for multiple scattering (Bourassa et al, 2008) and a non-linear relaxation inversion to retrieve profiles of ozone number density from 10 to 60 km altitudes with approximately 2 km vertical resolution and successive samples about every 500 km along the polar orbit track .…”
Section: Data Set Descriptionsmentioning
confidence: 99%
“…The optical spectrograph measures limb scattered sunlight at 280-810 nm, with a ∼ 1 nm spectral resolution. A review of the first decade of OSIRIS measurements is given by McLinden et al (2012).…”
Section: The Osiris Ozone Data Set From 2001 To the Presentmentioning
confidence: 99%