activity
20092025
most citedA generalized two-component model of solar wind turbulence and ab initio diffusion mean free paths and drift lengthscales of cosmic rays

62 citations · 624 across the 31 of their papers we have counts for

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Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2025★ 1 cited

Magnetohydrodynamic turbulence and the associated spatial diffusion tensor of cosmic rays in dynamical galactic halos

J. Kleimann, H. Fichtner, M. Stein +3

A detailed understanding of cosmic-ray transport in galactic halos is essential for explaining various observations, such as the radio continuum measurements of synchrotron radiati…

astro-ph.GA2025★ 6 cited

CHANG-ES XXXIV: Magnetic Field Structure in Edge-On Galaxies Characterising large-scale magnetic fields in galactic halos

M. Stein, J. Kleimann, B. Adebahr +12

Understanding galactic magnetic fields is essential for interpreting feedback processes in galaxies. Despite their importance, the exact structure of these fields, particularly in…

astro-ph.GA2021★ 20 cited

Simulating observable structures due to a perturbed interstellar medium in front of astrospheric bow shocks in 3D MHD

Lennart R. Baalmann, Klaus Scherer, Jens Kleimann +3

Context. While the shapes of many observed bow shocks can be reproduced by simple astrosphere models, more elaborate approaches have recently been used to explain differing observa…

astro-ph.GA2018★ 23 cited

Solenoidal Improvements for the JF12 Galactic Magnetic Field Model

Jens Kleimann, Timo Schorlepp, Lukas Merten +1

The popular JF12 analytic model by Jansson & Farrar provides a quantitative description of the Galaxy's large-scale magnetic field, which is widely used in various astrophysical ap…

astro-ph.GA2009★ 37 cited

Local Turbulence Simulations for the Multiphase ISM

R. Kissmann, J. Kleimann, H. Fichtner +1

In this paper we show results of numerical simulations for the turbulence in the interstellar medium. These results were obtained using a Riemann solver-free numerical scheme for h…