2014
DOI: 10.5194/amt-7-49-2014
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Assessment of Odin-OSIRIS ozone measurements from 2001 to the present using MLS, GOMOS, and ozonesondes

Abstract: Abstract. The Optical Spectrograph and InfraRed Imaging System (OSIRIS) was launched aboard the Odin satellite in 2001 and is continuing to take limb-scattered sunlight measurements of the atmosphere. This work aims to characterize and assess the stability of the OSIRIS 11 yr v5.0x ozone data set. Three validation data sets were used: the v2.2 Microwave Limb Sounder (MLS) and v6 Global Ozone Monitoring by Occultation of Stars (GOMOS) satellite data records, and ozonesonde measurements. Global mean percent diff… Show more

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Cited by 40 publications
(50 citation statements)
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“…Degenstein et al (2009) showed the version 5 data to be valid to 2 % down to 18 km by comparisons with SAGE II. The version 5.07 data (available at ftp://odin-osiris.usask.ca/Level2/daily) have been validated most recently and extensively by Adams et al (2013Adams et al ( , 2014. In the tropical upper troposphere, version 5 biases vs. ozonesondes and aircraft observations reach + 5 % (Cooper et al, 2011).…”
Section: Osirismentioning
confidence: 99%
See 1 more Smart Citation
“…Degenstein et al (2009) showed the version 5 data to be valid to 2 % down to 18 km by comparisons with SAGE II. The version 5.07 data (available at ftp://odin-osiris.usask.ca/Level2/daily) have been validated most recently and extensively by Adams et al (2013Adams et al ( , 2014. In the tropical upper troposphere, version 5 biases vs. ozonesondes and aircraft observations reach + 5 % (Cooper et al, 2011).…”
Section: Osirismentioning
confidence: 99%
“…For OSIRIS, we include only the observations made in the descending node of the orbit to avoid a scattering angle dependence of the retrieved ozone arising from residual aerosol interference that, if neglected, could lead to a trend in ozone as the proportion of ascending and descending node observations has changed over the mission lifetime. The Equator-crossing time in the descending and ascending nodes is ∼ 06:30/∼ 18:30, respectively (McLinden et al, 2012;Adams et al, 2014) having slightly precessed from 06:00/18:00. , resulting in no recent equatorial measurements in the ascending node.…”
Section: Osirismentioning
confidence: 99%
“…To date, three single-instrument extensions have been made to the SAGE-II record. These include one case extended with limb-scattered measurements from OSIRIS (Optical Spectrograph and Infrared Imager System) onboard the Odin satellite (2001-present) Adams et al, 2014;Sioris et al, 2014) and two cases using the stellar occultation measurements from GOMOS …”
Section: Sage-based Data Setsmentioning
confidence: 99%
“…They also noted that the long-term stability of OSIRIS up to 2012 was assessed by Adams et al (2014) using comparisons between OSIRIS, GOMOS, the Microwave Limb Sounder (MLS), and ozonesondes. This analysis showed that the OSIRIS data product did show some regions of positive drift (meaning higher ozone values) with respect to the other data sets, particularly after 2010; however, the global average drifts were < 3 % per decade between approximately 18 and 45 km.…”
Section: Introductionmentioning
confidence: 99%