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On the relationship between secular brightness changes of Titan and solar variability
Author(s) -
Pollack James B.,
Rages Kathy,
Toon Owen B.,
Yung Yuk L.
Publication year - 1980
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/gl007i010p00829
Subject(s) - brightness , titan (rocket family) , atmospheric sciences , secular variation , radiative transfer , environmental science , physics , astrobiology , astronomy , optics
Titan’ geometric albedo varied noticeably from 1972 to 1978, in phase with variations in solar activity [Lockwood and Thompson, 1979]. We carry out a series of radiative transfer and aerosol formation calculations in order to demonstrate the feasibility of the following scenario for these secular brightness changes: solar activity changes, especially in the UV output of the Sun, result in alterations to the mass production rate of aerosols in Titan’s atmosphere, which lead to modifications of their microphysical properties. The latter, in turn, cause the albedo to vary. Current estimates of the change in the solar UV radiation below the dissociation limit of methane imply alterations to the mean radius of the aerosols over an 11‐yr solar cycle that are consistent in sign and magnitude with those required to explain the observed secular brightness changes.