Open AccessReconstruction of three‐dimensional ozone fields using POAM III during SOLVE
Author(s) -
Randall C. E.,
Lumpe J. D.,
Bevilacqua R. M.,
Hoppel K. W.,
Fromm M. D.,
Salawitch R. J.,
Swartz W. H.,
Lloyd S. A.,
Kyro E.,
von der Gathen P.,
Claude H.,
Davies J.,
DeBacker H.,
Dier H.,
Molyneux M. J.,
Sancho J.
Publication year - 2002
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2001jd000471
Subject(s) - occultation , ozone , atmospheric sciences , environmental science , potential vorticity , aerosol , northern hemisphere , polar , middle latitudes , ozone layer , latitude , mixing ratio , meteorology , stratosphere , vorticity , geology , vortex , physics , geodesy , astronomy
In this paper we demonstrate the utility of the Polar Ozone and Aerosol Measurement (POAM) III data for providing semiglobal three‐dimensional ozone fields during the Stratospheric Aerosol and Gas Experiment (SAGE) III Ozone Loss and Validation Experiment (SOLVE) winter. As a solar occultation instrument, POAM III measurements were limited to latitudes of 63°N to 68°N during the SOLVE campaign but covered a wide range of potential vorticity. Using established mapping techniques, we have used the relation between potential vorticity and ozone measured by POAM III to calculate three‐dimensional ozone mixing ratio fields throughout the Northern Hemisphere on a daily basis during the 1999/2000 winter. To validate the results, we have extensively compared profiles obtained from ozonesondes and the Halogen Occultation Experiment to the proxy O 3 interpolated horizontally and vertically to the correlative measurement locations. On average, the proxy O 3 agrees with the correlative observations to better than ∼5%, at potential temperatures below about 900 K and latitudes above about 30°N, demonstrating the reliability of the reconstructed O 3 fields in these regions. We discuss the application of the POAM proxy ozone profiles for calculating photolysis rates along the ER‐2 and DC‐8 flight tracks during the SOLVE campaign, and we present a qualitative picture of the evolution of polar stratospheric ozone throughout the winter.