Abstract
The salient features of ionospheric scintillations at VHF at a station near the crest of the equatorial anomaly in India are derived from observations during 1987 to 1991, a period of rising solar activity. Predictions by a model due to Aarons /1/ of the nocturnal, seasonal and solar activity dependence of scintillation intensity are compared to observations at Rajkot. It is concluded that Aarons' model needs being modified for application in India.
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.
