Abstract
A PREREQUISITE for ionospheric work with satellites by means of the Doppler method is the knowledge of the behaviour of the Doppler-frequency shift in free space. A free-space condition prevails, if the operating frequency f is much greater than the maximum plasma frequency. It is the purpose of this communication to present in a general form an equation from which the minimum range between a satellite S and an observer P can be determined and to illustrate the magnitudes of higher-order terms.
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
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.
