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20022008
most citedECHO: an Eulerian Conservative High Order scheme for general relativistic magnetohydrodynamics and magnetodynamics

318 citations · 575 across the 5 of their papers we have counts for

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Showing 2004Show all

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astro-ph2004

Relativistic MHD simulations of pulsar bow-shock nebulae

N. Bucciantini, E. Amato, L. Del Zanna

Pulsar bow-shock nebulae are a class of pulsar wind nebulae (PWNe) that form when the pulsar wind is confined by the ram pressure of the ambient medium, and are usually associated…

astro-ph2004

Transverse oscillations in solar coronal loops induced by propagating Alfvenic pulses

Luca Del Zanna, Eveline Schaekens, Marco Velli

The propagation and the evolution of Alfvenic pulses in the solar coronal arcades is investigated by means of MHD numerical simulations. Significant transverse oscillations in coro…

astro-ph2004

Magnetic Rayleigh-Taylor instability for Pulsar Wind Nebulae in expanding Supernova Remnants

N. Bucciantini, E. Amato, R. Bandiera +2

We present a numerical investigation of the development of Rayleigh-Taylor instability at the interface between an expanding Pulsar Wind Nebula and its surrounding Supernova Remnan…

astro-ph2004

Axially symmetric relativistic MHD simulations of Pulsar Wind Nebulae in Supernova Remnants - On the origin of torus and jet-like features

L. Del Zanna, E. Amato, N. Bucciantini

The structure and the evolution of Pulsar Wind Nebulae (PWNe) are studied by means of two-dimensional axisymmetric relativistic magnetohydrodynamic (RMHD) simulations. After the fi…

astro-ph2004

The effects of spin-down on the structure and evolution of pulsar wind nebulae

N. Bucciantini, R. Bandiera, J. M. Blondin +2

We present high resolution spherically symmetric relativistic magnetohydrodynamical simulations of the evolution of a pulsar wind nebula inside the free expanding ejecta of the sup…