Abstract

An anisotropic magnetized plasma, in which the distribution of particle velocities is a bi-Maxwellian characterized by the temperatures ${T}_{\ensuremath{\perp}}$ and ${T}_{\mathrm{II}}$, is considered in order to delimit as much as possible the location of possibly unstable roots to the dispersion equation. We find that marginally unstable roots of the dispersion equation can occur only if both $[l+\frac{1}{2}]l\ensuremath{\omega}l[l+1\ensuremath{-}(\frac{{T}_{\mathrm{II}}}{{T}_{\ensuremath{\perp}}})]$ and $\ensuremath{\omega}l\frac{({T}_{\ensuremath{\perp}}\ensuremath{-}{T}_{\mathrm{II}})}{{T}_{\mathrm{II}}}$, where $l$ is an integer and $\ensuremath{\omega}$ is the real part of the frequency in units of the cyclotron frequency. Thus, in particular, the system is stable if ${T}_{\ensuremath{\perp}}l2{T}_{\mathrm{II}}$.

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 call

Disclaimer: 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.