activity
20102016
most citedOn numerical turbulence generation for test-particle simulations

41 citations · 181 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2016★ 27 cited

Application of the three-dimensional telegraph equation to cosmic-ray transport

R. C. Tautz, I. Lerche

An analytical solution to the the three-dimensional telegraph equation is presented. This equation has recently received some attention but so far the treatment has been one-dimens…

astro-ph.HE2016★ 1 cited

On the ergodicity of perpendicular cosmic ray transport

R. C. Tautz

Aims. The random walk of energetic charged particles in turbulent magnetic fields is investigated. Special focus is placed on transport across the mean magnetic field, which had be…

astro-ph.HE2015★ 6 cited

Monte-Carlo simulations of intensity profiles for energetic particle propagation

R. C. Tautz, J. Bolte, A. Shalchi

Aims. Numerical test-particle simulations are a reliable and frequently used tool to test analytical transport theories and to predict mean-free paths. The comparison between solut…

astro-ph.HE2015

Cosmic-ray acceleration at collisionless astrophysical shocks using Monte-Carlo simulations

M. Wolff, R. C. Tautz

Context. The diffusive shock acceleration mechanism has been widely accepted as the acceleration mechanism for galactic cosmic rays. While self-consistent hybrid simulations have s…

astro-ph.HE2015

Cosmic-ray diffusion in magnetized turbulence

R. C. Tautz

The problem of cosmic-ray scattering in the turbulent electromagnetic fields of the interstellar medium and the solar wind is of great importance due to the variety of applications…

astro-ph.HE2014★ 12 cited

Pitch-angle scattering of energetic particles with adiabatic focusing

R. C. Tautz, A. Shalchi, A. Dosch

Understanding turbulent transport of charged particles in magnetized plasmas often requires a model for the description of random variations in the particle's pitch angle. The Fokk…

astro-ph.HE2013★ 9 cited

Pitch-angle scattering in magnetostatic turbulence. II. Analytical considerations and pitch-angle isotropization

R. C. Tautz

Aims. The process of pitch-angle isotropization is important for many applications ranging from diffusive shock acceleration to large-scale cosmic-ray transport. Here, the basic an…

astro-ph.HE2013★ 19 cited

Pitch-angle scattering in magnetostatic turbulence. I. Test-particle simulations and the validity of analytical results

R. C. Tautz, A. Dosch, F. Effenberger +2

Context. Spacecraft observations have motivated the need for a refined description of the phase-space distribution function. Of particular importance is the pitch-angle diffusion c…

astro-ph.HE2013★ 4 cited

Interstellar Turbulent Magnetic Field Generation by Plasma Instabilities

R. C. Tautz, J. Triptow

The maximum magnetic field strength generated by Weibel-type plasma instabilities is estimated for typical conditions in the interstellar medium. The relevant kinetic dispersion re…

astro-ph.HE2013★ 5 cited

Modification of cosmic-ray energy spectra by stochastic acceleration

R. C. Tautz, I. Lerche, F. Kruse

Context: Typical space plasmas contain spatially and temporally variable turbulent electromagnetic fields. Understanding the transport of energetic particles and the acceleration m…

astro-ph.HE2013★ 41 cited

On numerical turbulence generation for test-particle simulations

R. C. Tautz, A. Dosch

A modified method is presented to generate artificial magnetic turbulence that is used for test-particle simulations. Such turbulent fields are obtained from the superposition of a…

physics.comp-ph2011★ 7 cited

On Simplified Numerical Turbulence Models in Test-particle Simulations

R. C. Tautz

Using the conventional approach of superposing plane waves, it is not possible to create a strictly isotropic turbulent magnetic field structure that obeys all physical constraints…

math-ph2011★ 11 cited

Methods for Summing General Kapteyn Series

R. C. Tautz, I. Lerche, D. Dominici

The general features and characteristics of Kapteyn series, which are a special type of series involving Bessel function, are investigated. For many applications to physics, astrop…

astro-ph.HE2010★ 29 cited

Simulating Heliospheric and Solar Particle Diffusion using the Parker Spiral Geometry

R. C. Tautz, A. Shalchi, A. Dosch

Cosmic Ray transport in curved background magnetic fields is investigated using numerical Monte-Carlo simulation techniques. Special emphasis is laid on the Solar system, where the…

astro-ph.HE2010★ 6 cited

A New Distribution Function for Relativistic Counterstreaming Plasmas

R. C. Tautz

The particle distribution function that describes two interpenetrating plasma streams is re-investigated. It is shown how, based on the Maxwell-Boltzmann-Jüttner distribution funct…

astro-ph.HE2010★ 4 cited

Non-linear Weibel-type Soliton Modes

R. C. Tautz, I. Lerche

Discussion is given of non-linear soliton behavior including coupling between electrostatic and electromagnetic potentials for non-relativistic, weakly relativistic, and fully rela…