Year-end Sale % OFF 
Abstract
We studied dynamics of a compact toroid in interplanetary space considering the diamagnetic force, gravity, and the drag force of the ambient solar wind. Magnetic cloud velocity profiles were calculated for different initial speeds using an expression of the diamagnetic force in purely toroidal coordinates.
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.
