activity
20052009
most citedAnisotropic Thermal Conduction and the Cooling Flow Problem in Galaxy Clusters

110 citations · 336 across the 6 of their papers we have counts for

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6 papers · 1 filter

astro-ph200867 cited

The Magnetothermal Instability in the Intracluster Medium

Ian J. Parrish, James M. Stone, M. Nicole Lemaster

The electron mean free path in the intracluster medium (ICM) of galaxy clusters is much larger than the gyroradius; thus, heat is transported anisotropically along magnetic field l…

astro-ph200777 cited

Nonlinear Simulations of the Heat Flux Driven Buoyancy Instability and its Implications for Galaxy Clusters

Ian J. Parrish, Eliot Quataert

In low collisionality plasmas heat flows almost exclusively along magnetic field lines, and the condition for stability to convection is modified from the standard Schwarzschild cr…

astro-ph20075 cited

Coulomb Bubbles: Over-stable Driving of Magnetoacoustic Waves Due to the Rapid and Anisotropic Diffusion of Energy

Aristotle Socrates, Ian J. Parrish, James M. Stone

We perform a linear magnetohydrodynamic perturbation analysis for a stratified magnetized envelope where the diffusion of heat is mediated by charged particles that are confined to…

astro-ph200672 cited

Saturation of the Magnetothermal Instability in Three Dimensions

Ian J. Parrish, James M. Stone

In dilute astrophysical plasmas, thermal conduction is primarily along magnetic field lines, and therefore highly anisotropic. As a result, the usual convective stability criterion…

astro-ph20065 cited

Simulation of the Magnetothermal Instability

Ian J. Parrish, James M. Stone

In many magnetized, dilute astrophysical plasmas, thermal conduction occurs almost exclusively parallel to magnetic field lines. In this case, the usual stability criterion for con…

astro-ph2005

Nonlinear Evolution of the Magnetothermal Instability in Two Dimensions

Ian J. Parrish, James M. Stone

In weakly magnetized, dilute plasmas in which thermal conduction along magnetic field lines is important, the usual convective stability criterion is modified. Instead of depending…