Making limb and nadir measurements comparable: A common volume study of PMC brightness observed by Odin OSIRIS and AIM CIPS

dc.bibliographicCitation.date2018
dc.bibliographicCitation.firstPage66
dc.bibliographicCitation.journalTitleJournal of atmospheric and solar-terrestrial physicseng
dc.bibliographicCitation.lastPage73
dc.bibliographicCitation.volume167
dc.contributor.authorBenze, Susanne
dc.contributor.authorGumbel, Jörg
dc.contributor.authorRandall, Cora E.
dc.contributor.authorKarlsson, Bodil
dc.contributor.authorHultgren, Kristoffer
dc.contributor.authorLumpe, Jerry D.
dc.contributor.authorBaumgarten, Gerd
dc.date.accessioned2022-12-20T13:23:14Z
dc.date.available2022-12-20T13:23:14Z
dc.date.issued2017
dc.description.abstractCombining limb and nadir satellite observations of Polar Mesospheric Clouds (PMCs) has long been recognized as problematic due to differences in observation geometry, scattering conditions, and retrieval approaches. This study offers a method of comparing PMC brightness observations from the nadir-viewing Aeronomy of Ice in the Mesosphere (AIM) Cloud Imaging and Particle Size (CIPS) instrument and the limb-viewing Odin Optical Spectrograph and InfraRed Imaging System (OSIRIS). OSIRIS and CIPS measurements are made comparable by defining a common volume for overlapping OSIRIS and CIPS observations for two northern hemisphere (NH) PMC seasons: NH08 and NH09. We define a scattering intensity quantity that is suitable for either nadir or limb observations and for different scattering conditions. A known CIPS bias is applied, differences in instrument sensitivity are analyzed and taken into account, and effects of cloud inhomogeneity and common volume definition on the comparison are discussed. Not accounting for instrument sensitivity differences or inhomogeneities in the PMC field, the mean relative difference in cloud brightness (CIPS - OSIRIS) is −102 ± 55%. The differences are largest for coincidences with very inhomogeneous clouds that are dominated by pixels that CIPS reports as non-cloud points. Removing these coincidences, the mean relative difference in cloud brightness reduces to −6 ± 14%. The correlation coefficient between the CIPS and OSIRIS measurements of PMC brightness variations in space and time is remarkably high, at 0.94. Overall, the comparison shows excellent agreement despite different retrieval approaches and observation geometries.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/10691
dc.identifier.urihttp://dx.doi.org/10.34657/9727
dc.language.isoeng
dc.publisherAmsterdam [u.a.] : Elsevier Science
dc.relation.doihttps://doi.org/10.1016/j.jastp.2017.11.007
dc.relation.essn1879-1824
dc.rights.licenseCC BY-NC-ND 4.0 Unported
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subject.ddc530
dc.subject.otherCIPSeng
dc.subject.otherCommon volumeeng
dc.subject.otherLimbeng
dc.subject.otherNadireng
dc.subject.otherOSIRISeng
dc.subject.otherPolar mesospheric cloudeng
dc.titleMaking limb and nadir measurements comparable: A common volume study of PMC brightness observed by Odin OSIRIS and AIM CIPSeng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorIAP
wgl.subjectPhysikger
wgl.typeZeitschriftenartikelger
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