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19972022
most citedThe Hall instability of thin weakly-ionized stratified Keplerian disks

17 citations · 177 across the 34 of their papers we have counts for

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7 papers · 1 filter

astro-ph2008★ 14 cited

Hall equilibrium of thin Keplerian disks embedded in mixed poloidal and toroidal magnetic fields

Yuri M. Shtemler, Michael Mond, Gunther Rudiger

Axisymmetric steady-state weakly ionized Hall-MHD Keplerian thin disks are investigated by using asymptotic expansions in the small disk aspect ratio ε. The model incorporates the…

astro-ph2008★ 14 cited

Evolution of initially localized perturbations in stratified ionized disks

Edward Liverts, Michael Mond

A detailed solution of an initial value problem of a vertically localized initial perturbation in rotating magnetized vertically stratified disk is presented. The appropriate linea…

astro-ph2008★ 2 cited

Current-driven instabilities in weakly ionized disks

Edward Liverts, Michael Mond, Vadim Urpin

Cool weakly ionized gaseous rotating disk form the basis for many models in astrophysics objects. Instabilities against perturbations in such disks play an important role in the th…

astro-ph2008★ 14 cited

The Tayler instability and the Hall effect in protoneutron stars

Guenther Ruediger, Manfred Schultz, Michael Mond +1

Collapse calculations indicate that the hot newly born protoneutron stars (PNS) rotate differentially so that strong toroidal magnetic field components should exist in the outer cr…

astro-ph2007★ 17 cited

The Hall instability of thin weakly-ionized stratified Keplerian disks

Yuri M. Shtemler, Michael Mond, Edward Liverts

The stratification-driven Hall instability in a weakly ionized polytropic plasma is investigated in the local approximation within an equilibrium Keplerian disk of a small aspect r…

astro-ph2007★ 14 cited

The Hall instability of weakly ionized, radially stratified, rotating disks

E. Liverts, M. Mond, A. D. Chernin

Cool weakly ionized gaseous rotating disk, are considered by many models as the origin of the evolution of protoplanetary clouds. Instabilities against perturbations in such disks…