Details of the Calculation of Upper
Tropospheric Humidity from the GOES Water Vapor Channel
The calculation of upper tropospheric humdity (UTH)
from satellite measurements is useful to monitor changes in water vapor
in the upper troposphere on a global and regional scale. The water vapor
transport index (WVTI) requires the calculation
of specific humidity to quantitatively represent moisture variations
in the upper layers of the atmosphere. Several methods have been
developed for retrieving upper tropospheric humidity (UTH) from
water vapor channel satellite measurements. Schmetz and Turpeinen
(1988) describe the operational algorithm in use by the European
Space Operations Centre (ESOC) for deriving UTH from METEOSAT
6.3-µm water vapor channel data. Their physical approach
employs radiative transfer calculations with European Centre
for Medium range Weather Forecast (ECMWF) temperature profile
data to generate look up tables to convert the water vapor radiances
to UTH. A modification to the approach (Schmetz et al. 1995a)
has been used for synoptic analysis of METEOSAT moisture data.
Soden and Bretherton (1993, 1996) also developed a technique for
converting water vapor brightness temperatures to UTH.
Simplified radiative transfer theory is used to arrive at their logrithmic
relationship between layer averaged humidity and the satellite brightness temperature. This approach
was originally developed for GOES-7 VAS water vapor measurements
and has since been applied to TIROS Operational Vertical Sounder
(TOVS) (e.g., Soden and Bretherton 1996; Stephens et al. 1996)
and Special Sensor Microwave Temperature (SSM/T2) (Spencer and
Braswell 1997) water vapor data. The approach used here is fundamentally
the same as SB96 but applied to GOES data with regression coefficients
derived on a monthly basis to account for temperature and humidity
variations not properly represented in a single set of regression
coefficients. In addition, the satellite zenith angle is explicitly
included in the equation derive the coefficients. For much of our work,
the NCEP monthly mean reanalysis (Kalnay et al. 1996) was used
to obtain Po and q, and saturation vapor pressure
over ice was used to get relative humidity. These Po
values are different from SB96 where climatological estimates
were used. Since the reanalysis model pressure level moisture
data extends only up to 300 hPa, relative humidity was decayed
exponentially above this level to satisfy the "weighting"
criteria in the SB96 technique. The model thermodynamic data
serves as input for the forward radiative transfer calculations
[transmittances calculated as in Weinreb (1981) with the GOES-7
6.7-mircometer channel spectral response function values] to generate
simulated channel brightness temperatures at each model grid
point. In the radiative transfer calculations, the satellite
zenith angle (based on a 0°N and 75°W satellite subpoint)
for each reanalysis model grid point (within the GOES-7 view
area of 60°N - 60°S and 0°-150°W) was used to
calculate a simulated VAS TB under non-nadir conditions. Simulated
brightness temperatures and the expression on the left side of
the humidity versus brightness temperature regression equation were used to investigate the relationship between the natural
logarithm of layer relative humidity and the water vapor brightness
temperature developed by SB96. The results of this analysis are
presented in figure. For relatively warm brightness temperatures
(TB > 235 K) the relationship is highly linear with minimal
scatter. Significant departure from a linear fit is observed
for zenith angles greater than 75° (red points). This seems
to be consistent with the other studies (Soden and Bretherton
1993, 1996; Schmetz et al 1995a; Spencer and Braswell 1997) although
specifics are lacking and consistent with Soden (1998b).
The relative humidity slope and intercept coefficients derived from
the monthly mean NCEP reanalysis data (2.5 x 2.5°) for 1988
with satellite zenith angles less than 75° using this procedure are
presented in the Table. The linear correlation coefficients between
TB and the left side of (4) are greater than about 0.95 for all
months. Although it may appear that an increase in the intercept
coefficient might be compensated for by a decrease in the slope
coefficient (as in the Boreal summer months), the retrieved humidity
is not the same in each case. To illustrate this point, two sets
of regression coefficients (January and July 1988) were applied
to a single day in June (June 14, 1988) and January (January
5, 1988) to demonstrate the effect of varying coefficients on
the humidity retrievals. The results are shown in the figure. A reversal
in the bias associated with using the wrong monthly coefficient
is evident for humidity below about 60%. For example, when using
July coefficients on January data (top chart in figure) in dry regions
(< 60% RH), the retrieved humidity is less moist (up to 10%
absolute difference). The opposite holds true when January coefficients
are applied to summer data (bottom chart). For relatively moist conditions
(> 60% RH) there is less of a bias but more scatter. These
figures therefore illustrate that summer coefficients applied
to winter data will enhance moisture gradients while winter coefficients
applied to summer data will tend to slightly weaken the humidity
gradients. This variation is undesirable. Therefore in our current
work coefficient scorresoponding to the current month are generated
and used to derive UTH. This approach
will may reduce retrieved relative humidity bias due to the use
of a single set of coefficients.
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Technical Contact: Dr. Gary J. Jedlovec (gary.jedlovec@msfc.nasa.gov)
Responsible Official: Dr. James L. Smoot (James.L.Smoot@nasa.gov)
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Last updated on: November 2, 1999 |