Abstract
The continuity and heat conduction equations for electrons, ions and neutral species are solved simultaneously from the viewpoint of studying the F-region magnetic storm behavior. It is shown that many of the observed changes in the F-region during the main phase of a magnetic storm can be successfully explained by assuming a decrease in oxygen concentration at the turbopause level. The specific changes in neutral composition, electron density, and electron, ion, and neutral temperatures during magnetic storms are discussed for different solar conditions.
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.
