We have calculated self-consistent equilibria of a collisionless relativistic
electron-positron gas in the vicinity of a magnetic $X-$point. For the
considered conditions, pertinent to extra-galactic jets, we find that leptons
are accelerated up to Lorentz factors $\Gamma_0 = \kappa e B_0L {\cal E}^2
/mc^2 \gg 1$, where $B_0$ is the typical magnetic field strength, ${\cal
E}\equiv E_0/B_0$, with $E_0$ the reconnection electric field, $L$ is the
length scale of the magnetic field, and $\kappa \approx 12$. The acceleration
is due to the dominance of the electric field over the magnetic field in a
region around the $X-$point. The distribution function of the accelerated
leptons is found to be approximately $dn/d\gamma \propto \gamma^{-1}$ for
$\gamma \lesssim \Gamma_0$. The apparent distribution function may be steeper
than $\gamma^{-1}$ due to the distribution of $\Gamma_0$ values and/or the
radiative losses. Self-consistent equilibria are found only for plasma inflow
rates to the $X-$point less than a critical value.Comment: submitted to ApJ; 6 figure
Non-circular tokamak plasmas can be unstable to ideal-MHD axisymmetric instabilities. Passive conductors with finite resistivity will at best slow down these instabilities to the resistive (L/R) time of the conductors. It is demonstrated that a simple active feedback system far from the plasma which responds on this resistive time can stabilize the system, provided its mutual inductance with the passive coils is small enough.
A pragmatic reanalysis of sleep disturbance data J. Acoust. Soc. Am. 118, 1888 (2005); 10.1121/1.4779605Re-analysis of the ultraviolet absorption spectrum of ozone
A comprehensive study of exponential-rigid-rotor equilibria, for strong electron and ion rings indicates the presence of a sizeable percentage of untrapped particles in all equilibria with aspect-ratios R/a ⪅ 4. Such aspect-ratios are required in fusion-relevant rings. Significant changes in the equilibria are observed when untrapped particles are excluded by the use of a truncated exponential-rigid-rotor distribution function.
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