Abstract
Abstract Topological pumping of the large-scale galactic magnetic field by the galactic fountain flow can be an important effect responsible for μG-strength magnetic fields in gaseous halos of spiral galaxies. The physical nature of this effect is discussed in application to spiral galaxies. In particular, we consider how topological pumping affects galactic dynamos and discuss specific properties of the large-scale galactic magnetic fields embedded in a turbulent flow of interstellar gas.
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.
