Atmospheric Chemistry and Physics Discussions
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10.5194/acpd-7-12097-2007
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http://www.atmos-chem-phys-discuss.net/7/12097/2007/acpd-7-12097-2007.pdf
12097
12143
2007-08-16
Ozone profile retrieval from limb scatter measurements in the HARTLEY bands: methodology, algorithm description, sensitivity studies, and validation
G. J. Rohen
rohen@iup.physik.uni-bremen.de
C. v. Savigny
J. W. Kaiser
E. J. Llewellyn
L. Froidevaux
M. López-Puertas
T. Steck
M. Palm
H. Winkler
J. P. Burrows
M. Sinnhuber
H. Bovensmann
Institute of Environmental Physics and Remote Sensing (IUP), Bremen, Germany
European Centre for Medium-Range Weather Forecasts (ECMWF), Reading, UK
Institute of Space and Atmospheric Studies (ISAS), Saskatoon, Canada
Jet Propulsion Laboratory (JPL), Pasadena, USA
Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain
Institut für Meteorologie und Klimaforschung (IMK), Karlsruhe-Leopoldshausen, Germany
SCIAMACHY limb scatter spectra have been used to retrieve atmospheric ozone
profiles in the upper stratosphere and lower mesosphere. Through a selection
of the wavelengths in the HARTLEY bands of ozone, profiles
extending to 60 or 70 km altitude were retrieved. This constitutes the
highest possible ozone profile information retrieval using the
backscatter technique.
<br><br>
Comparisons with profiles measured by a ground based radiometer in
Norway, MIPAS on board ENVISAT, HALOE on UARS and MLS on
AURA indicate a good agreement of the ozone profiles in the upper
stratosphere within 10% but also an increasing overestimation above
50 to 55 km.
<br><br>
Sensitivity studies show that solar zenith uncertainty and tangent
height errors are the largest error sources. Although the
tangent height is corrected through an own retrieval the correction
seemed to be be worser with increasing altitude and remains therefore as the
largest error source for this presented profile retrieval.
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