Abstract
The Periodic Multi-Sun-Synchronous Orbit allows the planning of observational cycles in which the solar illumination of the observed planet varies regularly, and returns to the initial condition at the beginning of each cycle. In the classical down-looking geometry of observation, this leads to the possibility of reconstructing the temporal evolution of all planetary parameters that are characterised by a typical variation in the solar day. In this paper, such an orbit is proposed to analyse the evolution of Mars’ atmosphere time-varying parameters taking into account, in addition to the down-looking configuration, a limb-looking geometry that works with a solar occultation technique.
Sign-in/Register to access full text options 
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 callDisclaimer: 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.
