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We present numerically calculated, disk--integrated, spectropolarimetricsignals of starlight that is reflected by vertically and horizontallyinhomogeneous gaseous exoplanets. We include various spatial features that arepresent on Solar System's gaseous planets: belts and zones, cyclonic spots, andpolar hazes, to test whether such features leave traces in the disk--integratedflux and polarization signals. Broadband flux and polarization signals ofstarlight that is reflected by gaseous exoplanets are calculated using anefficient, adding--doubling radiative transfer code, that fully includes singleand multiple scattering and polarization. The planetary model atmospheres arevertically inhomogeneous and can be horizontally inhomogeneous, and contain gasmolecules and/or cloud and/or aerosol particles.

Flux and polarization signals of spatially inhomogeneous gaseous exoplanets