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Accomplishments in FY02
The HES will be an infrared Michelson interferometer or grating
Atmospheric Infrared Sounder (AIRS) like sounder. Figure 1 shows
the spectral coverage of the current GOES sounder bands, 3-waveband
ABS, 2-waveband HES (ABS prime in the figure) and 2-waveband GIFTS
spectra. HES radiance measurements, at varying spectral resolutions,
can be converted into atmospheric temperature, moisture and ozone
profiles. HES spectral resolution will resolve individual carbon
dioxide absorption lines and should provide the high vertical resolution
soundings with the required accuracy.
Fast forward model development and retrieval algorithm developmentA new computationally efficient clear sky transmittance and radiance model has been developed for the HES spectral regions and resolution. This includes algorithms for computing clear sky transmission profiles and top-of-atmosphere radiance spectra, as well as fast tangent linear (Jacobian) model. The new fast model is based on new LBLRTM version and updated HITRAN 2000 spectroscopy data with local zenith angle extended to 70o (it was 650 in the old model). Figure 2 shows improved water vapor line parameters in CO2 region, LBL RTM calculation versus observation with HIS instrument.
An efficient algorithm for retrieving atmospheric temperature and moisture profiles from HES two waveband radiances has been updated with the new fast forward model. This algorithm regression procedure with all spectral channels followed by a nonlinear iterative physical approach using optimally selected channels. To perform the regression retrieval, HES radiances are calculated from the radiosonde observations of the atmospheric state, and the regression coefficients are generated from these calculated radiances/atmospheric profile pairs. The radiative transfer calculation of the ABS/HES two waveband spectral radiances is performed using the fast transmittance model mentioned above; this model has 101 pressure level vertical coordinates from 0.05 to 1100 hPa. The calculations take into account the satellite zenith angle, absorption by well-mixed gases (including nitrogen, oxygen, and carbon dioxide), water vapor (including the water vapor continuum), and ozone. The temperature and moisture sounding retrievals are produced when the regression coefficients are applied to the actual clear sky HES measurements. The advantage of this approach is that it does not need HES radiances collocated in time and space with atmospheric profile data, it requires only historical profile observations. This statistical regression algorithm is computationally efficient, numerically stable, and simple. In order to account for the nonlinearity of atmospheric parameter
to the HES radiances, a nonlinear iterative physical retrieval
procedure name regularization method along with the discrepancy
principle has been developed (Li and Huang 1999; Li et al. 2000,
Zhou et al. 2002) for hyperspectral infrared sounder data process.
This physical retrieval procedure uses the regression result as
a first guess for further profile modification.Fast and accurate
computation of Jacobian is very important for real time sounding
retrieval from HES data or near real time assimilation of HES radiances
in Numerical Weather Prediction (NWP). Two fast ways (analytical
form and transmittance ratio form, Li 1996) to compute the Jacobian
for HES forward model are tested and implemented in the physical
retrieval procedure. The Jacobian computation is radative transfer
model (RTM) model independent in the IR region; the computation
time is less than 2 brightness temperature (BT) calculations. Figure
3 shows water vapor mixing ratio weighting functions for HES 2-band
short midwave (SMW) band (1650 - 2250 cm-1) and the
current GOES sounder, along with the HES SMW brightness temperature
spectra. HES has much more vertical water vapor information in
troposphere than current GOES sounder. Because HES has two or three
bands that contain more than 1600 channels; it is not necessary
to use all channels in the physical retrieval processing. A subset
of channels (optimal channels) can be selected for the physical
retrieval process, the reasons for HES channel selection are: (a)
There are information redundancies among all the HES channels;
the other channels can represent some channels? information; (b)
The weighting function and inverse computation is very time consuming
in each iteration by use of all channels, a set of optimal channels
will significantly reduce the retrieval processing time and meet
the real time data processing requirement. Initial channel selection
has been tested in the physical retrieval procedure.
Retrieval trade-off studies with updated TRD noiseTrade-off studies were carried out. For example, when one spectral band fails or is too noisy for a given pixel, another one band only retrieval is tested against two-band altogether retrieval. The impact of reduced or increased instrument noise on retrieval is tested. Also, the impact of LW cutoff 685 cm-1 (GIFTS) versus 650 cm-1 on retrieval performance was studied.
Figure 5 shows the simulated 1km temperature retrieval RMSE from HES longwave 650cm-1 cutoff and 685cm-1 cutoff with the same TRD instrument noise, along with the simulated temperature retrieval RMSE from the current GOES sounder radiances. About 0.2 K improvement for upper tropospheric temperature is obtained with 650cm-1 cutoff over the 685cm-1 cutoff which GIFTS LW band starts. Figure 6 shows the 1km vertical temperature retrieval RMSE (left
panel) and 2km vertical water vapor (RH) retrieval RMSE (right
panel) from HES LW (650 - 1200 cm-1) only, SMW (1650
- 2250 cm-1) only, LW + SMW, and current GOES sounder.
It can be seen that temperature information is mostly provided
by LW only. For moisture information, LW provides very useful boundary
layer information while SMW provides most water vapor information
above 700 hPa, LW + SMW gives the best moisture vertical information.
HES two band TRD noise is added in the ABS/HES simulation. Figure
7 shows 1km vertical temperature retrieval RMSE (left panel) and
2km vertical water vapor (RH) retrieval RMSE (right panel) from
HES LW+ SMW with noise factor equal to 0.5 (half noise), 1.0 (TRD
noise) and 2.0 (double noise). It can be seen that the retrieval
error is almost linearly amplified by increased instrument noise.This
demonstrates that pixels with good noise performance will have
good sounding retrieval.
Initial ABS/HES algorithm validation using AIRS measurementsHES algorithm validation is being tested using Aqua's Atmospheric Infrared Sounder (AIRS) radiance measurements to ensure the operational purpose of the algorithm. ABS/HES algorithm has been adjusted to AIRS fast forward model for AIRS measurements retrieval processing. Routine AIRS data was first made available during the fall of 2002. Progress is undergoing for comparisons between AIRS retrievals and GOES products.Impact of band-to-band co-registration error on sounding retrieval from HESIn order to quantify the impact of band-to-band co-registration error on various sounding retrieval from HES 10km spatial resolution radiances. The MODIS 1km IR bands are used to compute band-to-band co-registration error with 10% (1km), 20% (2km) and 50% (5km) within 10km box area. The errors of MODIS IR bands are spectrally interpolated to ABS two-band spectra. Then this band-to-band co-registration error is added in the ABS/HES simulation. The upper panel of Figure 8 shows HES two wavebands? LW TRD noise and the errors with 10%, 20% and 50% band-band mis-alignment (or mis-registration), all the noises are scaled to NeDT@250K, while the lower panel show the brightness temperature spectra calculated from standard atmosphere.
The upper panel of Figure 8 shows HES two wavebands' SMW TRD noise
and the errors with 10%, 20% and 50% band-band mis-alignment, all
the noises are scaled to NeDT@250K. The lower panel shows the brightness
temperature spectra calculated from standard atmosphere.
Figure 9 is the same as Figure 8 but for SMW band.
Figure 10 shows the 1km vertical temperature and 2km RH retrieval RMSE from HES two-band simulation with 0% (no mis-alignment error), 10%, 20% and 50% band-band mis-alignment errors from LW band only. It can be seen that LW mis-alignment error will affect temperature and boundary layer moisture retrievals. Figure 11 shows the 1km vertical temperature and 2km RH retrieval RMSE from HES 2-band simulation with 0% (no mis-alignment error), 10%, 20% and 50% band-band mis-alignment errors from SMW band only. It can be seen that SMW mis-alignment error will only slightly affect temperature and boundary layer moisture retrievals. HES simulation study using CUBE data from MM5In order to demonstrate the capability of high temporal resolution HES on monitoring the evolution of weather system. The atmospheric cube data from MM5 has been created for the simulation study. The time step for the successive cube data is half hour, temperature and moisture regression retrievals (currently no physical retrieval in this cube study) are created from simulated HES clear radiances with TRD noise added, retrieval fields are compared with true atmospheric fields from the cubes to demonstrate the spatial and temporal characteristics of HES radiances and sounding retrievals.
Figure 12 shows simulated HES clear 700hPa water vapor mixing
ratio retrieval image (upper panel), true image (middle panel)
and the difference between retrieval and true (lower panel) at
time 1. Figure 13 is the same as Figure 12 but for time 2. The
HES TRD noise is added in the simulated radiances, only regression
approach is used in this cube study.
Cloud property retrieval from HES cloudy radiancesDue to the high spectral resolution the CO2 region, HES provides much more cloud property information than the current GOES spectral broad CO2 bands. Figure 14 shows HES 2-band LW cloud pressure sensitivity spectra with a cloud top pressure (CTP) of 200, 300, 500, 700 and 850hPa as a function of effective cloud amount (ECA) or effective cloud emissivity. Four panels show the calculations from 4 different atmospheric states.
To compare the HES and the current GOES sounder cloud parameter retrievals, a simulation study was conducted. A set of 75 CONUS radiosonde profiles, that represent different atmospheric conditions. Twenty combinations were formed from each profile by assigning two CTPs plus 50 hPa random variation (200 hPa and 300 hPa corresponding to very high-, high-level clouds) and 10 ECAs (0.1, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9 and 1.0). The HES and GOES-8 longwave spectral band cloudy radiances were simulated for all combinations of each profile. An infrared surface emissivity of 0.98 for each longwave spectral band was assumed in the simulation. The HES TRD noise and GOES-8 instrument noise were added into cloudy radiance. Cloud retrievals from both ABS/HES with local minimum emissivity variance (LMEV, Huang et al. 2002) and GOES-8 sounder with 1DVAR (Li et al. 2001) are compared with true CTPs for RMSE calculations. In order to account for the surface uncertainties and the atmospheric profile error in the LMEV and 1DVAR cloud retrievals, nominal errors were considered in the simulation. For atmospheric temperature, a 1.5 K random error was assumed at each pressure level, which is close to the accuracy of the forecast analysis. For surface skin temperature a nominal random error of 2.5 K was assumed in the simulation. In addition, 1.0% error was included for infrared (IR) surface emissivity and 15% error was included for water vapor mixing ratio at each pressure level. Figure 15 shows the simulated HES and current GOES sounder CTP retrieval RMSE as a function of effective cloud amount (ECA) or effective cloud emissivity. For thin clouds, high spectral is very important for more accurate clouds. Conclusions from FY02 accomplishment
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