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Title: Intercomparison of slant column measurements of NO[subscript 2] and O[subscript 4] by MAX-DOAS and zenith-sky UV and visible spectrometers
Authors: Roscoe, H.K.
Van Roozendael M.
Fayt, C.
du Piesanie A.
Abuhassan, N.
Adams, C.
Akrami, M.
Cede, A.
Chong, J.
Clemer, K.
Friess, U.
Ojeda, M.G.
Goutail, F.
Graves, R.
Griesfeller, A.
Grossmann, K.
Hemerijckx, G.
Hendrick, F.
Herman, J.
Hermans, C.
Irie, H.
Johnston, P.V.
Kanaya, Y.
Kreher, K.
Leigh, R.
Merlaud, A.
Mount, G.H.
Navarro, M.
Oetjen, H.
Pazmino, A.
Perez-Camacho, M.
Peters, E.
Pinardi, G.
Puentedura, O.
Richter, A.
Schoenhardt, A.
Shaiganfar, R.
Spinei, E.
Strong, K.
Takashima, H.
Vlemmix, T.
Vrekoussis, M.
Wagner, T.
Wittrock, F.
Yela, M.
Yilmaz, S.
Boersma, F.
Hains, J.
Kroon, M.
Piters, A.
Kim, Y.J.
First Published: 2010
Publisher: European Geosciences Union (EGU) and COPERNICUS GESELLSCHAFT MBH
Citation: ATMOSPHERIC MEASUREMENT TECHNIQUES, 2010, 3 (6), pp. 1629-1646
Abstract: In June 2009, 22 spectrometers from 14 institutes measured tropospheric and stratospheric NO[subscript 2] from the ground for more than 11 days during the Cabauw Intercomparison Campaign of Nitrogen Dioxide measuring Instruments (CINDI), at Cabauw, NL (51.97° N, 4.93° E). All visible instruments used a common wavelength range and set of cross sections for the spectral analysis. Most of the instruments were of the multi-axis design with analysis by differential spectroscopy software (MAX-DOAS), whose non-zenith slant columns were compared by examining slopes of their least-squares straight line fits to mean values of a selection of instruments, after taking 30-min averages. Zenith slant columns near twilight were compared by fits to interpolated values of a reference instrument, then normalised by the mean of the slopes of the best instruments. For visible MAX-DOAS instruments, the means of the fitted slopes for NO[subscript 2] and O[subscript 4] of all except one instrument were within 10% of unity at almost all non-zenith elevations, and most were within 5%. Values for UV MAX-DOAS instruments were almost as good, being 12% and 7%, respectively. For visible instruments at zenith near twilight, the means of the fitted slopes of all instruments were within 5% of unity. This level of agreement is as good as that of previous intercomparisons, despite the site not being ideal for zenith twilight measurements. It bodes well for the future of measurements of tropospheric NO[subscript 2], as previous intercomparisons were only for zenith instruments focussing on stratospheric NO[subscript 2], with their longer heritage.
DOI Link: 10.5194/amt-3-1629-2010
ISSN: 1867-1381
eISSN: 1867-8548
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2010 The authors. This is an open-access article distributed under the terms of the Creative Commons Attribution License (, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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