Abstract
A cross-field instability is considered in a magnetized, dusty plasma acted upon by a gravity field, g , perpendicular to the magnetic field, B , permeating the plasma. Waves are produced traveling essentially with the dust grains zero-order motion. The condition for excitation of the instability is that the dust zero-order velocity perpendicular to both g and B exceed the dust-acoustic speed, C da . Numerical results are presented for an ionospheric type plasma and for a laboratory type plasma.
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.
