Abstract
Based on long-term spectrophotometric observations of Jupiter in the wavelength range 320–1100 nm, we investigate the variations of aerosol extinction (at λ 320–600 nm) and methane–ammonia absorption (at λ 600–1100 nm) over Jupiter's disk. We give estimates of the optical parameters for the upper cloud layer of the planet, the overlying stratospheric haze, and a Rayleigh atmosphere.
Published Version
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have