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dc.contributor.author
Wiegner, Matthias
dc.contributor.author
Mattis, Ina
dc.contributor.author
Pattantyús-Ábrahám, Margit
dc.contributor.author
Bravo-Aranda, Juan Antonio
dc.contributor.author
Poltera, Yann
dc.contributor.author
Haefele, Alexander
dc.contributor.author
Hervo, Maxime
dc.contributor.author
Görsdorf, Ulrich
dc.contributor.author
Leinweber, Ronny
dc.contributor.author
Gasteiger, Josef
dc.contributor.author
Haeffelin, Martial
dc.contributor.author
Wagner, Frank
dc.contributor.author
Cermak, Jan
dc.contributor.author
Komínková, Katerina
dc.contributor.author
Brettle, Mike
dc.contributor.author
Münkel, Christoph
dc.contributor.author
Pönitz, Kornelia
dc.date.accessioned
2019-02-18T17:17:11Z
dc.date.available
2019-02-03T04:32:46Z
dc.date.available
2019-02-18T17:17:11Z
dc.date.issued
2019-01-25
dc.identifier.issn
1867-1381
dc.identifier.issn
1867-8548
dc.identifier.other
10.5194/amt-12-471-2019
en_US
dc.identifier.uri
http://hdl.handle.net/20.500.11850/322761
dc.identifier.doi
10.3929/ethz-b-000322761
dc.description.abstract
With the rapidly growing number of automated single-wavelength backscatter lidars (ceilometers), their potential benefit for aerosol remote sensing received considerable scientific attention. When studying the accuracy of retrieved particle backscatter coefficients, it must be considered that most of the ceilometers are influenced by water vapor absorption in the spectral range around 910 nm. In the literature methodologies have been proposed to correct for this effect; however, a validation was not yet performed. In the framework of the ceilometer intercomparison campaign CeiLinEx2015 in Lindenberg, Germany, hosted by the German Weather Service, it was possible to tackle this open issue. Ceilometers from Lufft (CHM15k and CHM15kx, operating at 1064 nm), from Vaisala (CL51 and CL31) and from Campbell Scientific (CS135), all operating at a wavelength of approximately 910 nm, were deployed together with a multi-wavelength research lidar (RALPH) that served as a reference. In this paper the validation of the water vapor correction is performed by comparing ceilometer backscatter signals with measurements of the reference system extrapolated to the water vapor regime. One inherent problem of the validation is the spectral extrapolation of particle optical properties. For this purpose AERONET measurements and inversions of RALPH signals were used. Another issue is that the vertical range where validation is possible is limited to the upper part of the mixing layer due to incomplete overlap and the generally low signal-to-noise ratio and signal artifacts above that layer. Our intercomparisons show that the water vapor correction leads to quite a good agreement between the extrapolated reference signal and the measurements in the case of CL51 ceilometers at one or more wavelengths in the specified range of the laser diode's emission. This ambiguity is due to the similar effective water vapor transmission at several wavelengths. In the case of CL31 and CS135 ceilometers the validation was not always successful. That suggests that error sources beyond the water vapor absorption might be dominant. For future applications we recommend monitoring the emitted wavelength and providing “dark” measurements on a regular basis.
en_US
dc.format
application/pdf
dc.language.iso
en
en_US
dc.publisher
Copernicus
en_US
dc.rights.uri
http://creativecommons.org/licenses/by/4.0/
dc.title
Aerosol backscatter profiles from ceilometers: Validation of water vapor correction in the framework of CeiLinEx2015
en_US
dc.type
Journal Article
dc.rights.license
Creative Commons Attribution 4.0 International
ethz.journal.title
Atmospheric Measurement Techniques
ethz.journal.volume
12
en_US
ethz.journal.issue
1
en_US
ethz.journal.abbreviated
Atmos. meas. tech.
ethz.pages.start
471
en_US
ethz.pages.end
490
en_US
ethz.version.deposit
publishedVersion
en_US
ethz.identifier.wos
ethz.identifier.scopus
ethz.publication.place
Göttingen
en_US
ethz.publication.status
published
en_US
ethz.date.deposited
2019-02-03T04:32:47Z
ethz.source
SCOPUS
ethz.eth
yes
en_US
ethz.availability
Open access
en_US
ethz.rosetta.installDate
2019-02-18T17:17:28Z
ethz.rosetta.lastUpdated
2021-02-15T03:39:21Z
ethz.rosetta.versionExported
true
ethz.COinS
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