&Dynamics and Physics of Bodies of the Solar System BRussian KJupiter, absorption coefficients of methane// We propose a modification of the method used before for the revision of monochromatic absorption coefficients in thermal conditions of Jupiter's atmosphere. Methane absorption bands over a wavelength interval from 441 to 940 nm were taken into account. We developed a method of allowing for high-altitude atmospheric temperature profile in the change of k_v for methane absorption bands formed at different penetration depths in the atmosphere.