Validation of 10-year SAO OMI Ozone Profile (PROFOZ) product using ozonesonde observations
We validate the Ozone Monitoring Instrument (OMI) Ozone Profile (PROFOZ) product from October 2004 through December 2014 retrieved by the Smithsonian Astrophysical Observatory (SAO) algorithm against ozonesonde observations. We also evaluate the effects of OMI row anomaly (RA) on the retrieval by...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2017-07-01
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Series: | Atmospheric Measurement Techniques |
Online Access: | https://www.atmos-meas-tech.net/10/2455/2017/amt-10-2455-2017.pdf |
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author | G. Huang X. Liu K. Chance K. Yang P. K. Bhartia Z. Cai M. Allaart G. Ancellet B. Calpini G. J. R. Coetzee E. Cuevas-Agulló M. Cupeiro H. De Backer M. K. Dubey H. E. Fuelberg M. Fujiwara S. Godin-Beekmann T. J. Hall B. Johnson E. Joseph R. Kivi B. Kois N. Komala G. König-Langlo G. Laneve T. Leblanc M. Marchand K. R. Minschwaner G. Morris M. J. Newchurch S.-Y. Ogino N. Ohkawara A. J. M. Piters F. Posny R. Querel R. Scheele F. J. Schmidlin R. C. Schnell O. Schrems H. Selkirk M. Shiotani P. Skrivánková R. Stübi G. Taha D. W. Tarasick A. M. Thompson V. Thouret M. B. Tully R. Van Malderen H. Vömel P. von der Gathen J. C. Witte M. Yela |
author_facet | G. Huang X. Liu K. Chance K. Yang P. K. Bhartia Z. Cai M. Allaart G. Ancellet B. Calpini G. J. R. Coetzee E. Cuevas-Agulló M. Cupeiro H. De Backer M. K. Dubey H. E. Fuelberg M. Fujiwara S. Godin-Beekmann T. J. Hall B. Johnson E. Joseph R. Kivi B. Kois N. Komala G. König-Langlo G. Laneve T. Leblanc M. Marchand K. R. Minschwaner G. Morris M. J. Newchurch S.-Y. Ogino N. Ohkawara A. J. M. Piters F. Posny R. Querel R. Scheele F. J. Schmidlin R. C. Schnell O. Schrems H. Selkirk M. Shiotani P. Skrivánková R. Stübi G. Taha D. W. Tarasick A. M. Thompson V. Thouret M. B. Tully R. Van Malderen H. Vömel P. von der Gathen J. C. Witte M. Yela |
author_sort | G. Huang |
collection | DOAJ |
description | We validate the Ozone Monitoring Instrument (OMI) Ozone Profile (PROFOZ)
product from October 2004 through December 2014 retrieved by the Smithsonian
Astrophysical Observatory (SAO) algorithm against ozonesonde observations. We
also evaluate the effects of OMI row anomaly (RA) on the retrieval by
dividing the dataset into before and after the occurrence of serious OMI RA,
i.e., pre-RA (2004–2008) and post-RA (2009–2014). The retrieval shows good
agreement with ozonesondes in the tropics and midlatitudes and for pressure
< ∼ 50 hPa in the high latitudes. It demonstrates clear improvement
over the a priori down to the lower troposphere in the tropics and down to an
average of ∼ 550 (300) hPa at middle (high) latitudes. In the tropics
and midlatitudes, the profile mean biases (MBs) are less than 6 %, and
the standard deviations (SDs) range from 5 to 10 % for pressure < ∼ 50 hPa to less than 18 % (27 %) in the tropics (midlatitudes)
for pressure > ∼ 50 hPa after applying OMI averaging kernels to
ozonesonde data. The MBs of the stratospheric ozone column (SOC, the ozone
column from the tropopause pressure to the ozonesonde burst pressure) are
within 2 % with SDs of < 5 % and the MBs of the tropospheric ozone
column (TOC) are within 6 % with SDs of 15 %. In the high latitudes,
the profile MBs are within 10 % with SDs of 5–15 % for pressure < ∼ 50 hPa but increase to 30 % with SDs as great as 40 % for
pressure > ∼ 50 hPa. The SOC MBs increase up to 3 % with SDs as
great as 6 % and the TOC SDs increase up to 30 %. The comparison
generally degrades at larger solar zenith angles (SZA) due to weaker signals
and additional sources of error, leading to worse performance at high
latitudes and during the midlatitude winter. Agreement also degrades with
increasing cloudiness for pressure > ∼ 100 hPa and varies with
cross-track position, especially with large MBs and SDs at extreme off-nadir
positions. In the tropics and midlatitudes, the post-RA comparison is
considerably worse with larger SDs reaching 2 % in the stratosphere and
8 % in the troposphere and up to 6 % in TOC. There are systematic
differences that vary with latitude compared to the pre-RA comparison. The
retrieval comparison demonstrates good long-term stability during the pre-RA
period but exhibits a statistically significant trend of
0.14–0.7 % year<sup>−1</sup> for pressure < ∼ 80 hPa,
0.7 DU year<sup>−1</sup> in SOC, and −0. 33 DU year<sup>−1</sup> in TOC during the
post-RA period. The spatiotemporal variation of retrieval performance
suggests the need to improve OMI's radiometric calibration especially during
the post-RA period to maintain the long-term stability and reduce the
latitude/season/SZA and cross-track dependency of retrieval quality. |
first_indexed | 2024-12-21T03:53:36Z |
format | Article |
id | doaj.art-17899fc72e7c457cbb608f237d7c8878 |
institution | Directory Open Access Journal |
issn | 1867-1381 1867-8548 |
language | English |
last_indexed | 2024-12-21T03:53:36Z |
publishDate | 2017-07-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Atmospheric Measurement Techniques |
spelling | doaj.art-17899fc72e7c457cbb608f237d7c88782022-12-21T19:16:54ZengCopernicus PublicationsAtmospheric Measurement Techniques1867-13811867-85482017-07-01102455247510.5194/amt-10-2455-2017Validation of 10-year SAO OMI Ozone Profile (PROFOZ) product using ozonesonde observationsG. Huang0X. Liu1K. Chance2K. Yang3P. K. Bhartia4Z. Cai5M. Allaart6G. Ancellet7B. Calpini8G. J. R. Coetzee9E. Cuevas-Agulló10M. Cupeiro11H. De Backer12M. K. Dubey13H. E. Fuelberg14M. Fujiwara15S. Godin-Beekmann16T. J. Hall17B. Johnson18E. Joseph19R. Kivi20B. Kois21N. Komala22G. König-Langlo23G. Laneve24T. Leblanc25M. Marchand26K. R. Minschwaner27G. Morris28M. J. Newchurch29S.-Y. Ogino30N. Ohkawara31A. J. M. Piters32F. Posny33R. Querel34R. Scheele35F. J. Schmidlin36R. C. Schnell37O. Schrems38H. Selkirk39M. Shiotani40P. Skrivánková41R. Stübi42G. Taha43D. W. Tarasick44A. M. Thompson45V. Thouret46M. B. Tully47R. Van Malderen48H. Vömel49P. von der Gathen50J. C. Witte51M. Yela52Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USAHarvard-Smithsonian Center for Astrophysics, Cambridge, MA, USAHarvard-Smithsonian Center for Astrophysics, Cambridge, MA, USADepartment of Atmospheric and Oceanic Science, University of Maryland, College Park, Maryland, USANASA Goddard Space Flight Center, Greenbelt, Maryland, USAHarvard-Smithsonian Center for Astrophysics, Cambridge, MA, USARoyal Netherlands Meteorological Institute (KNMI), De Bilt, the NetherlandsLATMOS-ISPL, Université Paris 6 Pierre-et-Marie-Curie, Paris, FranceMeteoSwiss Aerological Station, Federal Office of Meteorology and Climatology MeteoSwiss, Payerne, SwitzerlandSouth African Weather Service, Pretoria, South AfricaIzana Atmospheric Research Center, Meteorological State Agency of Spain, Santa Cruz de Tenerife, SpainNational Meteorological Service, Ushuaia, Tierra del Fuego, ArgentinaRoyal Meteorological Institute of Belgium, Brussels, BelgiumLos Alamos National Laboratory, Los Alamos, NM, USAEarth, Ocean and Atmospheric Sciences, Florida State University, Tallahassee, FL, USAFaculty of Environmental Earth Science, Hokkaido University, Sapporo, JapanLATMOS-ISPL, Université Paris 6 Pierre-et-Marie-Curie, Paris, FranceEarth, Ocean and Atmospheric Sciences, Florida State University, Tallahassee, FL, USANOAA/ESRL Global Monitoring Division, Boulder, CO, USAAtmospheric Sciences Research Center, SUNY at Albany, Albany, NY, USAFinnish Meteorological Institute, Sodankylä, FinlandThe Institute of Meteorology and Water Management, National Research Institute, Warsaw, PolandIndonesian Institute of Aeronautics and Space (LAPAN), Bandung, IndonesiaAlfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, Bremerhaven, GermanyEarth Observation Satellite Images Applications Lab (EOSIAL), Università di Roma “La Sapienza”, Rome, ItalyJet Propulsion Laboratory, California Institute of Technology, Wrightwood, CA, USALATMOS-ISPL, Université Paris 6 Pierre-et-Marie-Curie, Paris, FranceDepartment of Physics, New Mexico Institute of Mining and Technology, Socorro, NM, USASt. Edward's University, Austin, TX, USADepartment of Atmospheric Science, University of Alabama in Huntsville, Huntsville, AL, USADepartment of Coupled Ocean-Atmosphere-Land Processes Research, Japan Agency for Marine-Earth Science and Technology, Yokosuka, JapanGlobal Environment and Marine Department, Japan Meteorological Agency, Tokyo, JapanRoyal Netherlands Meteorological Institute (KNMI), De Bilt, the NetherlandsUniversité de la Réunion, Saint Denis, FranceNational Institute of Water and Atmospheric Research, Lauder, Central Otago, New ZealandRoyal Netherlands Meteorological Institute (KNMI), De Bilt, the NetherlandsNASA Goddard Space Flight Center, Greenbelt, Maryland, USANOAA/ESRL Global Monitoring Division, Boulder, CO, USAAlfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, Bremerhaven, GermanyUniversities Space Research Association, Greenbelt, MD, USAResearch Institute for Sustainable Humanosphere, Kyoto University, Kyoto, JapanUpper Air and Surface Observation Department, Czech Hydrometeorological Institute, Prague, Czech RepublicMeteoSwiss Aerological Station, Federal Office of Meteorology and Climatology MeteoSwiss, Payerne, SwitzerlandUniversities Space Research Association, Greenbelt, MD, USAAir Quality Research Division, Environment & Climate Change Canada, Downsview, ON, CanadaNASA Goddard Space Flight Center, Greenbelt, Maryland, USALaboratoire d'Aérologie, Université de Toulouse, CNRS, UPS, Toulouse, FranceBureau of Meteorology, Melbourne, Victoria, AustraliaRoyal Meteorological Institute of Belgium, Brussels, BelgiumEarth Observing Laboratory, National Center for Atmospheric Research, Boulder, CO, USAAlfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, Potsdam, GermanyScience Systems and Applications Inc., Greenbelt, MD, USAAtmospheric Research and Instrumentation Branch, National Institute for Aerospace Technology (INTA), Madrid, SpainWe validate the Ozone Monitoring Instrument (OMI) Ozone Profile (PROFOZ) product from October 2004 through December 2014 retrieved by the Smithsonian Astrophysical Observatory (SAO) algorithm against ozonesonde observations. We also evaluate the effects of OMI row anomaly (RA) on the retrieval by dividing the dataset into before and after the occurrence of serious OMI RA, i.e., pre-RA (2004–2008) and post-RA (2009–2014). The retrieval shows good agreement with ozonesondes in the tropics and midlatitudes and for pressure < ∼ 50 hPa in the high latitudes. It demonstrates clear improvement over the a priori down to the lower troposphere in the tropics and down to an average of ∼ 550 (300) hPa at middle (high) latitudes. In the tropics and midlatitudes, the profile mean biases (MBs) are less than 6 %, and the standard deviations (SDs) range from 5 to 10 % for pressure < ∼ 50 hPa to less than 18 % (27 %) in the tropics (midlatitudes) for pressure > ∼ 50 hPa after applying OMI averaging kernels to ozonesonde data. The MBs of the stratospheric ozone column (SOC, the ozone column from the tropopause pressure to the ozonesonde burst pressure) are within 2 % with SDs of < 5 % and the MBs of the tropospheric ozone column (TOC) are within 6 % with SDs of 15 %. In the high latitudes, the profile MBs are within 10 % with SDs of 5–15 % for pressure < ∼ 50 hPa but increase to 30 % with SDs as great as 40 % for pressure > ∼ 50 hPa. The SOC MBs increase up to 3 % with SDs as great as 6 % and the TOC SDs increase up to 30 %. The comparison generally degrades at larger solar zenith angles (SZA) due to weaker signals and additional sources of error, leading to worse performance at high latitudes and during the midlatitude winter. Agreement also degrades with increasing cloudiness for pressure > ∼ 100 hPa and varies with cross-track position, especially with large MBs and SDs at extreme off-nadir positions. In the tropics and midlatitudes, the post-RA comparison is considerably worse with larger SDs reaching 2 % in the stratosphere and 8 % in the troposphere and up to 6 % in TOC. There are systematic differences that vary with latitude compared to the pre-RA comparison. The retrieval comparison demonstrates good long-term stability during the pre-RA period but exhibits a statistically significant trend of 0.14–0.7 % year<sup>−1</sup> for pressure < ∼ 80 hPa, 0.7 DU year<sup>−1</sup> in SOC, and −0. 33 DU year<sup>−1</sup> in TOC during the post-RA period. The spatiotemporal variation of retrieval performance suggests the need to improve OMI's radiometric calibration especially during the post-RA period to maintain the long-term stability and reduce the latitude/season/SZA and cross-track dependency of retrieval quality.https://www.atmos-meas-tech.net/10/2455/2017/amt-10-2455-2017.pdf |
spellingShingle | G. Huang X. Liu K. Chance K. Yang P. K. Bhartia Z. Cai M. Allaart G. Ancellet B. Calpini G. J. R. Coetzee E. Cuevas-Agulló M. Cupeiro H. De Backer M. K. Dubey H. E. Fuelberg M. Fujiwara S. Godin-Beekmann T. J. Hall B. Johnson E. Joseph R. Kivi B. Kois N. Komala G. König-Langlo G. Laneve T. Leblanc M. Marchand K. R. Minschwaner G. Morris M. J. Newchurch S.-Y. Ogino N. Ohkawara A. J. M. Piters F. Posny R. Querel R. Scheele F. J. Schmidlin R. C. Schnell O. Schrems H. Selkirk M. Shiotani P. Skrivánková R. Stübi G. Taha D. W. Tarasick A. M. Thompson V. Thouret M. B. Tully R. Van Malderen H. Vömel P. von der Gathen J. C. Witte M. Yela Validation of 10-year SAO OMI Ozone Profile (PROFOZ) product using ozonesonde observations Atmospheric Measurement Techniques |
title | Validation of 10-year SAO OMI Ozone Profile (PROFOZ) product using ozonesonde observations |
title_full | Validation of 10-year SAO OMI Ozone Profile (PROFOZ) product using ozonesonde observations |
title_fullStr | Validation of 10-year SAO OMI Ozone Profile (PROFOZ) product using ozonesonde observations |
title_full_unstemmed | Validation of 10-year SAO OMI Ozone Profile (PROFOZ) product using ozonesonde observations |
title_short | Validation of 10-year SAO OMI Ozone Profile (PROFOZ) product using ozonesonde observations |
title_sort | validation of 10 year sao omi ozone profile profoz product using ozonesonde observations |
url | https://www.atmos-meas-tech.net/10/2455/2017/amt-10-2455-2017.pdf |
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