Abstract

Using the spectrophotometric measurements data of 2015, the relation of values of the imaginary part n i of aerosol refractive index was determined for latitudinal belts 17° N, 33° N, 49° N, and 66° N of Saturn’s disc. A steadily decreasing tendency in the relative n i values when moving northward from the equatorial region of the disk to the latitude 49° N, inclusive, was revealed. The n i values in the 17° N and 49° N belts were found to differ significantly from other latitudinal regions of the giant planet’s disk.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.