Infrared sounders represent some of the most sophisticated instruments used in Earth and planetary observation. These instruments measure thermal infrared radiation emitted by Earth's atmosphere and surface to obtain vertical temperature and humidity profiles, composition of various atmospheric gases, cloud properties, and surface characteristics. This article provides an overview of infrared sounder data processing techniques and their applications.
Infrared sounders measure the upwelling thermal radiation from the Earth-atmosphere system in multiple spectral bands. These measurements contain information about the vertical structure of atmospheric temperature and humidity profiles, as well as concentrations of trace gases such as ozone, carbon monoxide, carbon dioxide, and methane.
Satellite infrared sounders have been operational since the 1970s, starting with the Vertical Temperature Profile Radiometer (VTPR) on NOAA satellites. Modern infrared sounders, such as the Atmospheric Infrared Sounder (AIRS) on NASA's Aqua satellite, the Infrared Atmospheric Sounding Interferometer (IASI) on MetOp satellites, and the Cross-track Infrared Sounder (CrIS) on NOAA's Suomi NPP and NOAA-20 satellites, provide thousands of spectral channels with high spectral resolution, enabling more accurate retrievals.
Infrared sounders typically operate in spectral ranges from approximately 660 to 2,800 cm (3.57-15.15 m), covering both shortwave and thermal infrared regions. Modern hyperspectral sounders like IASI and CrIS are based on Fourier transform interferometry, providing thousands of spectral channels with fine spectral resolution (0.25-0.5 cm).
Key instrument parameters affecting data processing include:
The first step in infrared sounder data processing is the acquisition of raw digital counts from the instrument. These raw measurements are converted to calibrated radiances through a series of preprocessing steps:
1. Dark signal subtraction: Remove instrument self-emission and detector dark current
2. Nonlinearity correction: Account for detector response nonlinearities
3. Radiometric calibration: Convert digital counts to radiances using onboard blackbody targets and space views
4. Spectral calibration: Correct for spectral registration and resolution effects
5. Geolocation: Assign precise latitude, longitude, and viewing geometry to each measurement
Modern sounders perform most of these calibrations onboard, but additional refinements are often applied in ground processing to improve accuracy.
The foundation of infrared sounder data processing is radiative transfer modeling, which describes how infrared radiation propagates through the atmosphere. The radiative transfer equation for infrared sounding can be expressed as:
R(v) = (v) B(v,T_s) (v,s) + B(v,T(z)) (v,z)/z dz
Where R(v) is the measured radiance at wavenumber v, (v) is surface emissivity, B(v,T) is the Planck function at temperature T, T_s is surface temperature, is atmospheric transmission, and the integral represents atmospheric contribution.
Accurate radiative transfer models must account for:
Laboratory-measured spectroscopic parameters from databases like HITRAN (High-Resolution Transmission Molecular Absorption Database) feed into radiative transfer calculation codes such as LBLRTM (Line-by-Line Radiative Transfer Model) and MODTRAN (Moderate Resolution Atmospheric Transmittance and Radiance Code).
Clouds significantly affect infrared sounder measurements, challenging the retrieval of atmospheric profiles. Cloud detection identifies measurements contaminated by clouds, while cloud clearing techniques attempt to extract clear-column radiances for partially cloudy fields of view.
Common cloud detection approaches include:
For partially cloudy scenes, cloud clearing algorithms such as the Atmospheric Infrared Sounder cloud clearing (NCE) and the Minimum Residual method combine information from multiple spectral channels and fields of view to estimate what the radiance would be in clear conditions.
Retrieval algorithms invert the measured radiances to estimate geophysical parameters of interest. This inversion problem is mathematically ill-posed, requiring regularization to stabilize the solution. Common retrieval approaches include:
Most operational infrared sounder retrievals use optimal estimation, which formally balances measurement information with prior expectations and provides uncertainty estimates:
x = x_a + KRK + R_a)KR(y - F(x_a))
Where x is the retrieved state, x_a is the a priori state, K is the Jacobian (sensitivity of radiances to state changes), R is the measurement error covariance, R_a is the a priori covariance, y is the measurement vector, and F(x) is the radiative transfer forward model.
Typical products derived from infrared sounder measurements include:
Quality control (QC) identifies and flags retrieval products that may have poor reliability. QC metrics include:
Validation compares retrieved products with independent measurements from radiosondes, aircraft, ground-based instruments, and other satellites to assess accuracy and identify systematic biases.
Infrared sounder data has revolutionized numerical weather prediction (NWP) through data assimilation. Rather than using retrieved profiles directly, modern NWP systems assimilate either calibrated radiances or retrieved products. The assimilation of clear-sky radiances from hyperspectral sounders like AIRS, IASI, and CrIS is estimated to have significantly improved forecast skill, particularly in the Southern Hemisphere where conventional observations are sparse.
Beyond weather forecasting, infrared sounders contribute to climate monitoring and environmental science:
The future of infrared sounding will focus on:
Infrared sounder data processing encompasses a complex chain of operations from raw measurements to geophysical parameters. Through advances in instrument technology, radiative transfer modeling, and retrieval algorithms, these systems provide invaluable information for weather forecasting, climate monitoring, and environmental science. As satellite technology and computational methods continue to evolve, we can expect even more accurate and comprehensive atmospheric information from future infrared sounders.
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