Over optically
thick cloud systems, presence of polarized signatures at 37 and 85 GHz is evidenced and analyzed with the help of cloud top temperature and optical thickness extracted from visible and IR satellite observations.
Not exact matches
That's because the
system is swaddled in a
thick cloud of charged particles shed from the companion star, and these particles scatter photons.
Based on the available data, the astronomers concluded that the planet's atmosphere is either a thin but dense layer rich in water steam or a
thick layer of high
clouds or hazes, similar to those seen in the atmospheres of Venus and Titan in the Solar
System.