Abstract
The fluctuation of the acceleration are analysed for several satellites. For the density variations three predominant influences can be distinguished: 1) The varying solar short ultra-violet radiation; 2) The day-night-effect; 3) An annual variation. The latter suggests a significant interaction of the terrestrial upper atmosphere with the interplanetary matter. The annual variation gives some evidence for an interstellar wind due to the solar motion in the local stellar system.
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.
