activity
20192022
most citedNo longer ballistic, not yet diffusive--the formation of cosmic ray small-scale anisotropies

11 citations · 16 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2022★ 2 cited

Diffusion of relativistic charged particles and field lines in isotropic turbulence: II. Analytical models

Marco Kuhlen, Vo Hong Minh Phan, Philipp Mertsch

The transport of high-energy particles in the presence of small-scale, turbulent magnetic fields is a long-standing issue in astrophysics. Analytical theories on transport perpendi…

astro-ph.HE2022★ 3 cited

Diffusion of relativistic charged particles and field lines in isotropic turbulence: I. Numerical simulations

Marco Kuhlen, Vo Hong Minh Phan, Philipp Mertsch

The transport of non-thermal particles across a large-scale magnetic field in the presence of magnetised turbulence has been a long-standing issue in high-energy astrophysics. Of p…

astro-ph.HE2021★ 11 cited

No longer ballistic, not yet diffusive--the formation of cosmic ray small-scale anisotropies

Marco Kuhlen, Vo Hong Minh Phan, Philipp Mertsch

The arrival directions of TeV-PeV cosmic rays are remarkably uniform due to the isotropization of their directions by scattering on turbulent magnetic fields. Small anisotropies ca…

astro-ph.HE2021

Cosmic Ray Small Scale Anisotropies in Slab Turbulence

Marco Kuhlen, Philipp Mertsch, Vo Hong Minh Phan

In the standard picture of cosmic ray transport the propagation of charged cosmic rays through turbulent magnetic fields is described as a random walk with cosmic rays scattering o…

astro-ph.HE2019

Time-dependent AMS-02 electron-positron fluxes in an extended force-field model

Marco Kuhlen, Philipp Mertsch

The magnetised solar wind modulates the Galactic cosmic ray flux in the heliosphere up to rigidities as high as 40 GeV. In this work, we present a new and straightforward extension…