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J. Kleimann

31 papers hereh-index 17618 citations61 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author7
  • middle author20
  • last author1

Across the 29 of 31 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR19
  • astro-ph.GA5
  • physics.space-ph4
  • astro-ph.HE2
  • astro-ph.IM1
same name
  • J. Kleimann — 2 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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

collaborators
Showing 2022Show all

3 papers · 1 filter

physics.space-ph2022★ 43 cited

Turbulence in the outer heliosphere

Federico Fraternale, Laxman Adhikari, Horst Fichtner +9

The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their interaction is governed by complex physical processes and creates heliospheric regions with sign…

astro-ph.SR2022★ 1 cited

An exact analytical solution for the weakly magnetized flow around an axially symmetric paraboloid, with application to magnetosphere models

Jens Kleimann, Christian Röken

Rotationally symmetric bodies with longitudinal cross sections of parabolic shape are frequently used to model astrophysical objects, such as magnetospheres and other blunt objects…

astro-ph.SR2022★ 7 cited

Modelling O-star astrospheres with different relative speeds between the ISM and the star: 2D and 3D MHD model comparison

L. R. Baalmann, K. Scherer, J. Kleimann +3

Context. State of the art simulations of astrospheres are modelled using three-dimensional (3D) magnetohydrodynamics (MHD). An astrospheric interaction of a stellar wind (SW) with…

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