Calibration Products

The AIRS calibration team provides two calibrated products, AIRS L1B and AIRS L1C. These data products are then used to create higher level data products.

AIRS data products figure, showing data flow relationships L2 & L3 products may have variations depending on data from subsets of AIRS, AMSU-A, or HSB. AIRS L0 (L0 are the raw bits from the spacecraft.) AIRS L0 -> AIRS L1A v5 (L1A Non-engineering data is not archived, but can be recreated from L0.) AIRS L1A v5 -> AIRS L1B v5 AIRS L1B v5 -> AIRS L1C v6.7 AIRS L1C v6.7 -> CHIRP v2 AIRS L1B v5 -> AIRS L2/L3 v6 AIRS L1B v5 -> AIRS L2/L3 v7 AIRS L1B v5 -> CLIMCAPS L2/L3 v2 AIRS L1B v5 -> JoSFRA (coming soon) AIRS L1B v5 & AIRS L1C v6.7 -> CalSub v2

The calibration data sets are found at the GES DISC:

Input Data Files Used for Calibration

Calibration of AIRS data depends on a small collection of input data files which describe the instrument performance. These files are provided here.

Spectral Response Functions

The Spectral Response Functions (SRFs) describe the wavelength at which each AIRS channel responds. The original preflight SRF data was measured with a Fourier Transform Spectrometer (FTS).

The L1B and L1C data products have separate SRF data sets, since the L1C channels are moved onto a regularly-spaced grid. The data files and descriptions are found at:


Strow, Larrabee L., et al. "Prelaunch spectral calibration of the Atmospheric Infrared Sounder (AIRS)." IEEE transactions on geoscience and remote sensing 41.2 (2003): 274-286.

Gaiser, Steven L., et al. "In-flight spectral calibration of the atmospheric infrared sounder." IEEE Transactions on Geoscience and Remote Sensing 41.2 (2003): 287-297.

Strow, L. L., et al. "Validation of the Atmospheric Infrared Sounder radiative transfer algorithm." Journal of Geophysical Research: Atmospheres 111.D9 (2006).

Point Spread Functions

Each individual sounding that AIRS does not measure a single ray through the atmosphere, but a bundle of rays. At any place in the atmosphere or on the ground, this bundle of rays appears as a circular patch, smeared by the side-to-side scanning and motion of the Aura spacecraft. These circular patches are not perfectly uniform, largely due to polarization effects inside the instrument. The point spread functions (PSFs) model this smeared patch. The PSFs are also known as "tophats," since the ground-based data as taken resembles a flat-topped cylinder when plotted in 3D.

Four images showing how the AIRS footprint is determined: a) Measured ‘top hat’ data from 1.1° circular mask data measured before flight. b) Cut to a width of 0.6° wide in spectral direction, since measured mask was with round mask. c) Rotated, due to scan mirror rotation effect. d) Smeared in the scan direction

The PSF data files are available on request.


Elliott, Denis A., Thomas S. Pagano, and H. H. Aumann. "The impact of the AIRS spatial response on channel-to-channel and multi-instrument data analyses." Earth Observing Systems XI 6296 (2006): 171-179.

Pagano, Thomas S., et al. "Improving AIRS radiance spectra in high contrast scenes using MODIS." Earth Observing Systems XX. Vol. 9607. SPIE, 2015.

Channel Properties Files

The channel properties and calibration properties files contain the current and past history of the instrument performance parameters needed for calibration. These files are periodically updated every few years and uploaded to the GES DISC. The file formats are human-readable text files.


Noise Covariance Matrix

The noise covariance matrix contains information on the relationship between the noise performance between pairs of spectrometer channels. In practice, only pairs of channels from the same module have meaningful correlation.

The noise covariance files are available on request.

AIRS Noise Covariance Matrix
AIRS Noise Covariance Matrix
AIRS Noise Covariance Matrix (K)
AIRS Noise Covariance Matrix (K)
AIRS NEdT (K) at 250 K
AIRS NEdT (K) at 250 K
AIRS NEdT (K) at 250 K
AIRS NEdT (K) at 250 K