Digital Earth Emissivity Information System (DEEIS) - JCSDA Algorithm
Physical Basis of Surface Emissivity Calculation from Satellite Observations
Satellite microwave measurements of brightness temperatures for a non-scattering atmosphere can be expressed as follows:
(1)With

where TB is the brightness temperatures at satellite height, e is the surface emissivity, Ts is the surface temperature, t the optical depth, z the atmospheric transmittance, m the cosine of the satellite local zenith angle; Tu and Td are the brightness temperatures associated with upwelling and downwelling radiations, respectively. Variables z, Tu, and Td can be obtained from the absorption model for given atmospheric profiles of temperature and water vapor.
For window channels, the atmospheric transmittance is near unity under clear conditions and high for non-precipitating conditions so that Tu and Td are small. This implies that satellite microwave measurements are strongly characterized by surface emissivity. However, although the atmospheric corrections are small for window channels, they still need to be accounted for. Using (1), the emissivity is given by:
(2)Since the radiation at the AMSU frequencies emanates from a thin surface layer, with penetration depths on the order of the wavelength, Eqs. (1) and (2) involve an “effective” emissivity over the depth of penetration and within the field of view of the satellite instrument.
SSMI Algorithm
Training Data Set
Direct microwave emissivity measurements are not available over various land
surface conditions. Thus, the "truth" emissivity is also derived from SSM/I measurements
of brightness temperatures. In doing so, the contributions to SSMI measurements from
the atmospheric emission and surface temperature are first removed using an emission-based
radiative transfer equation:
(1)According to our analyses, the errors in various source terms in Eq. (1) (e.g., surface temperature, brightness temperature and transmittance) result in the errors in derived emissivity. In particular, one percent of error in the surface temperature would result in less than one percent error in land emissivity. The error due to water vapor results in the largest error in emissivity at 22V that is located at the water vapor absorption line. Prigent et al. (1997) estimated the range of these errors: with a typical value of 0.6 K the radiometric noise in measured brightness temperature will induce only small uncertainties on the emissivity retrieval using Eq. (1); with a value of 4 K in the surface temperature, the uncertainty is about 0.024; with a uncertainty of 30 % in moisture profile, the uncertainty in emissivity distributes between 0.001 and 0.02 at both 19.35, and 37.0 GHz and 0.005 and 0.1 at both 22.235 and 85.5 GHz. It is believed that our training data set of the emissivity may contain similar uncertainty.
Regression Algorithm Formula
With the multiple regression method, land emissivity at an SSM/I channel is predicted using seven channel
SSM/I brightness temperatures as
(2)| ε1 | ε2 | ε3 | ε4 | ε5 | ε6 | ε7 | |
|---|---|---|---|---|---|---|---|
| a0 | -1.20E-01 | -1.45E-01 | -1.02E-01 | -2.16E-01 | -2.08E-01 | -2.31E-01 | -2.63E-01 |
| a11 | 5.57E-03 | 8.55E-04 | -3.00E-03 | -1.05E-03 | -2.01E-03 | -4.99E-03 | -6.45E-03 |
| a12 | 2.98E-06 | 5.46E-06 | 1.93E-05 | 7.75E-06 | 1.07E-05 | 2.30E-05 | 3.02E-05 |
| a13 | 7.05E-01 | 1.15E-02 | 9.81E-03 | 7.21E-03 | 7.05E-03 | 9.97E-03 | 1.08E-02 |
| a14 | -1.44E-05 | -1.57E-05 | -2.21E-05 | -1.44E-05 | -1.45E-05 | -2.21E-05 | -2.49E-05 |
| a15 | -3.59E-03 | -3.57E-03 | 1.54E-03 | -3.98E-03 | -3.20E-03 | -3.19E-03 | -2.28E-03 |
| a16 | -9.27E-06 | -9.88E-06 | -1.87E-05 | -8.78E-06 | -1.10E-05 | -1.92E-05 | -2.55E-05 |
| a17 | 2.63E-03 | 2.25E-03 | 2.33E-03 | 9.97E-03 | 4.85E-03 | 5.86E-03 | 4.15E-03 |
| a21 | 1.17E-06 | 9.04E-07 | 1.84E-06 | -4.00E-06 | -3.37E-06 | -4.48E-06 | -1.13E-06 |
| a22 | -3.78E-03 | -3.19E-03 | -3.83E-03 | -3.96E-03 | 1.39E-03 | -4.40E-03 | -3.04E-03 |
| a23 | 7.37E-06 | 7.23E-06 | 9.78E-06 | 7.09E-06 | 6.08E-06 | 1.02E-05 | 9.00E-06 |
| a24 | 7.06E-03 | 5.16E-03 | 9.56E-03 | 7.85E-03 | 5.85E-03 | 1.24E-02 | 1.05E-02 |
| a25 | -1.66E-05 | -1.15E-05 | -2.18E-05 | -1.88E-05 | -1.36E-05 | -1.73E-05 | -2.35E-05 |
| a26 | -7.09E-03 | -5.02E-03 | -8.43E-03 | -7.60E-03 | -5.58E-03 | -6.78E-03 | -4.34E-03 |
| a27 | 1.40E-05 | 8.35E-06 | 1.59E-05 | 1.56E-05 | 1.02E-05 | 1.23E-05 | 1.73E-05 |
Statistical Results of Emissivity Errors
With Eq. (2) and the coefficients given in Table 1, the emissivity at seven SSM/I channels can be rieved over various land conditions.
Note that the outliers of some SSM/I pixels away from 1:1 line may be related to the snow conditions here the algorithm may overestimate the emissivity. The predicted noises are also produced by the presence of clouds that cannot be detected from SSM/I brightness temperatures. Figure 1 is a comparison between the emissivity predicted using Eq. (2) and the truth using Eq. (1). It is found that the standard deviation is about 0.02 at 19.35 and 37 GHz and about 0.03 at 22.235 and 85.5 GHz, and the errors are larger at 22.235 and 85.5 GHz due to stronger water vapor absorption. At 85.5 GHz, cloud liquid water produces additional errors.



