The Optimised Retrieval
Model (ORM) performs in near real time the
retrieval of pressure, temperature and volume mixing ratio of six
high-priority species, namely O3, H2O, HNO3,
CH4, N2O and NO2.
The retrieval strategy of ORM is based upon the following three choices:
1
Use of ‘microwindows’
The redundancy of
information coming from MIPAS measurements
makes it possible to select a set of narrow (less than 3 cm-1 width)
spectral intervals containing the best information on the target
parameters, while the intervals containing little or no information can
be ignored. The use of selected spectral intervals, called
‘microwindows’, allows the size of analyzed spectral elements to be
limited and avoids the analysis of spectral regions more affected by
systematic errors.
2
Sequential retrieval of the species
The unknowns are
retrieved using the following sequence of
operations. First temperature and ‘tangent pressures’ are retrieved
simultaneously, then the target species volume mixing ratio profiles
are retrieved individually in sequence. The reason of this approach is
that a simultaneous retrieval of all the species would require a huge
amount of computer memory, because the size of the matrices to be
handled by the retrieval is proportional to the product between the
unknown parameters and the number of observations. The sequence of the
target species retrieval has been determined according to the degree of
their reciprocal spectral interference and is: H2O, O3,
HNO3, CH4, N2O
and NO2.
3 Global
fit analysis of the limb scanning sequence
A global fit approach is
adopted for the retrieval of each
vertical profile. This means that spectral data relating to a complete
limb scan sequence are fitted simultaneously. The global fit provides a
comprehensive exploitation of the information and a rigorous
determination of the correlations between atmospheric parameters at the
different altitudes. Besides, it permits the full exploitation of
hydrostatic equilibrium condition and is better compatible with the
modelling of the finite field of view of the instrument.
The ORM code has been developed by the Earth Observation group of
IFAC-CNR (Firenze - Italy) in collaboration with the Department of
Physical and Inorganic Chemistry - University of Bologna (Bologna -
Italy), the ISAC-CNR (Bologna - Italy), the IMK (Karlsruhe - Germany),
LPMA (Paris - France), University of Oxford and University of
Leicester. The ESA study for the development of the ORM covered the
years 1995 - 2002.
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