Abstract
To determine the aerosol absorption component of the effective optical depth τ κeff , a special method has been developed. It is based on the implausible effect of the decrease of the aerosol scattering component τ aeff in dependence on the atmospheric pressure P, if τ κeff = 0. It is the elimination of this effect by selecting the values of τ κeff that allows the latter to be determined. This method was tested with the data of observations of the North Equatorial Belt (NEB) of Jupiter’s disk in the methane absorption bands at λ = 619 and 727 nm. This allowed us to determine the values of τ κeff and the imaginary part of the refractive index of aerosol particles (n i = 0.00063, 0.00065, 0.0007, and 0.00069 at λ = 605.5, 631.3, 714.7, and 741.4 nm, respectively) and to correctly specify the characteristic of the vertical structure of clouds of the planet.
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Original Russian Text © A.V. Morozhenko, A.S. Ovsak, 2015, published in Kinematika i Fizika Nebesnykh Tel, 2015, Vol. 31, No. 5, pp. 20–29.
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Morozhenko, A.V., Ovsak, A.S. On the possibility of separation of aerosol and methane absorption in the long-wavelength spectral range for giant planets. Kinemat. Phys. Celest. Bodies 31, 225–231 (2015). https://doi.org/10.3103/S0884591315050074
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DOI: https://doi.org/10.3103/S0884591315050074