Wednesday, 12 January 2000
In early November 1994, during the ATLAS-3
space-shuttle mission, the Atmospheric Trace
Molecule Spectroscopy (ATMOS) instrument made
measurements of many trace gases, including
ozone. Ozone observations for this time
period are available from four other satellite
instruments: the Upper Atmosphere Research
Satellite (UARS) Halogen Occultation Experiment
(HALOE), the UARS Microwave Limb Sounder
(MLS), the Polar Ozone and Aerosol Measurement
(POAM II), and the Stratospheric Aerosol and
Gas Experiment (SAGE II). Data from ATMOS
and several of the other instruments have
recently been reprocessed with new retrieval
software versions. We compare observations from
these five satellite instruments in potential
vorticity (PV) coordinates by mapping the
ozone observations during the ATLAS-3 period
in Equivalent Latitude/theta space, as well
as showing profile comparisons with the usual
coincidence criteria augmented by requiring
coincidence in potential vorticity. Reasons for
discrepencies in Equivalent Latitude/theta maps
of ozone related to the different sampling
patterns of the instruments are discussed.
High-resolution trajectory profile calculations
are used to show the origins of laminated
structures in ozone profiles from several
instruments.
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