Spectral response functions

Spectral response functions (SRFs) and MW passbands

If you have information on updates or corrections to any of the spectral response function or pass band information below, please let us know either on the RTTOV forum or via the NWP SAF Helpdesk.

All coefficient files for a particular instrument (e.g. those based on different predictor versions or supporting different variable gases) use the same SRF data.

The channels for each instrument are listed in the coefficient file order. You can confirm the RTTOV channel order by looking at the coefficient file headers or by using the rttov_coef_info.exe tool.

The README_SRF section is copied from the coefficient files at the top of each page linked below.


Spectral response functions for VIS/IR coefficient files

(A)ATSR

ABI

AGRI

AHI

AMI

ASTER

AVHRR

CLIM

ECOSTRESS

EOIR
Unable to publish due to restrictions.

EPIC

FCI

GMS IMAGER

GOES IMAGER

GOES SOUNDER

HIRS

HIRS-shifted

HRIR

IIR

INSAT-3D(R/S) IMAGER

INSAT-3D(R/S) SOUNDER

IRAS

IRMSS

LI

  • MTG 1 LI – SRFs cannot be published due to licence restrictions

LSTM

MBFIRI

MERSI-1

MERSI-2

MERSI-LL

  • FY-3E MERSI-LL – SRFs cannot be published due to licence restrictions

MERSI-3

MERSI-RM

METIMAGE

MI

MODIS

MRIR

Earth-CARE MSI

Sentinel-2 MSI

MSUGS

MSUMR

MTSAT IMAGER

MVIRI (IR channels)

MVIRI (VIS channel)

MVISR

OLCI

OLI

NASA SBG

SEVIRI

SGLI

SIRS

SLSTR

SSH

OceanSat SSTM

THIR

TIRS

TM

TRISHNA-TIR

VIIRS

VIMS

VIRR

VISSR

VTPR


Spectral response data for MW coefficient files

Full spectral response function data are available for a subset of microwave sensors. The corresponding optical depth coefficient files include “_srf” in the filenames.

Pass band data for MW coefficient files

Most MW coefficient files are based on “top-hat” (or “box-car”) spectral responses. These are defined in plain ASCII “filter files”. The filter files have been updated with a new file format in 2025. The nominal top-hat specification for any given sensor is common to that instrument on all platforms, but there is now one filter file per individual sensor as the files now contain additional information specific to each individual instrument. The file headers describe the contents.