activity
19992024
most citedMPI-AMRVAC 2.0 for Solar and Astrophysical Applications

250 citations · 5.3k across the 118 of their papers we have counts for

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Showing 2013Show all

6 papers · 1 filter

astro-ph.HE2013★ 32 cited

Relativistic 3D jet simulations for the X-ray binary SS433

Remi Monceau-Baroux, Rony Keppens, Zakaria Meliani +1

Context. Modern high resolution observations allow to view closer into the objects powering relativistic jets. This is especially the case for SS433, an X-ray binary from which a p…

astro-ph.SR2013★ 61 cited

3D Prominence-hosting Magnetic Configurations: Creating a Helical Magnetic Flux Rope

Chun Xia, Rony Keppens, Yang Guo

The magnetic configuration hosting prominences and their surrounding coro- nal structure is a key research topic in solar physics. Recent theoretical and observational studies stro…

astro-ph.GA2013★ 19 cited

Relativistic AGN jets II. Jet properties and mixing effects for episodic jet activity

Sander Walg, Abraham Achterberg, Sera Markoff +2

Various radio galaxies show signs of having gone through episodic jet outbursts in the past. An example is the class of double-double radio galaxies (DDRGs). However, to follow the…

physics.space-ph2013★ 60 cited

Nonlinear evolution of the magnetized Kelvin-Helmholtz instability: from fluid to kinetic modeling

P. Henri, S. S. Cerri, F. Califano +11

The nonlinear evolution of collisionless plasmas is typically a multi-scale process where the energy is injected at large, fluid scales and dissipated at small, kinetic scales. Acc…

astro-ph.HE2013★ 206 cited

Three-Dimensional Magnetohydrodynamic Simulations of the Crab Nebula

Oliver Porth, Serguei S. Komissarov, Rony Keppens

In this paper we give a detailed account of the first 3D relativistic magnetohydrodynamic (MHD) simulations of Pulsar Wind Nebulae (PWN), with parameters most suitable for the Crab…

astro-ph.SR2013★ 65 cited

Parametric survey of longitudinal prominence oscillation simulations

Q. M. Zhang, P. F. Chen, C. Xia +2

It is found that both microflare-sized impulsive heating at one leg of the loop and a suddenly imposed velocity perturbation can propel the prominence to oscillate along the magnet…