source:
tapas/web/resources/doc/infosResolution_en.txt
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| 1 | The user must enter the resolution power, defined as λ/FWHM. TAPAS computes the FWHM, and the atmospheric transmission will be convolved by a Gaussian with this specific FWHM. Note that the FWHM is changing with wavelength or wave number, since the spectral resolution is defined as a unit-less number. It is constant in wave number units within small intervals defined inside the LBLRTM computation. |
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