activity
20092025
most citedHeliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields

82 citations · 1.3k across the 57 of their papers we have counts for

collaborators

57 papers

astro-ph.HE2025★ 11 cited

Relativistic regularized kappa distributions

Linh Han Than, Klaus Scherer, Horst Fichtner

The special relativistic generalization of isotropic regularized kappa distributions is derived and compared to that of the original Olbertian (or standard) kappa distributions. It…

physics.plasm-ph2023

Electron Holes in a Regularized Kappa Background

Fernando Haas, Horst Fichtner, Klaus Scherer

The pseudopotential method is used to derive electron hole structures in a suprathermal plasma having a regularized probability distribution function background. The regularize…

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.HE2022★ 2 cited

Implications from 3D modeling of gamma-ray signatures in the Galactic Center Region

J. Becker Tjus, P. -S. Blomenkamp, J. Dörner +4

Context. The Galactic Center (GC) region has been studied in gamma rays in the past decades - the GC excess detected by Fermi is still not fully understood and the first detection…

astro-ph.SR2022

On the properties of 0.11 keV to 344 MeV ion spectra in the inner heliosheath using regularized -distributions

Klaus Scherer, Kostas Dialynas, Horst Fichtner +2

The shape of the ion energy spectra plays a critical role toward determining the ion energetics, the acceleration mechanisms and the possible sources of different plasma and suprat…

astro-ph.SR2022

Revisiting the Ulysses electron data with a triple fit of velocity distributions

Klaus Scherer, Edin Husidic, Marian Lazar +1

Given their uniqueness, the Ulysses data can still provide us with valuable new clues about the properties of plasma populations in the solar wind, and, especially, about their var…

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…

physics.plasm-ph2022★ 8 cited

Towards a realistic evaluation of transport coefficients in non-equilibrium space plasmas

Edin Husidic, Klaus Scherer, Marian Lazar +2

Recent studies have outlined the interest for the evaluation of transport coefficients in space plasmas, where the observed velocity distributions of plasma particles are condition…

astro-ph.HE2021

Implications of turbulence-dependent diffusion on cosmic-ray spectra

J. Dörner, P. Reichherzer, L. Merten +4

The propagation of cosmic rays can be described as a diffusive motion in most galactic environments. High-energy gamma-rays measured by Fermi have allowed inference of a gradient i…

astro-ph.SR2021

An Exact, Time-dependent Analytical Solution for the Magnetic Field in the Inner Heliosheath

Christian Röken, Jens Kleimann, Horst Fichtner

We derive an exact, time-dependent analytical magnetic field solution for the inner heliosheath, which satisfies both the induction equation of ideal magnetohydrodynamics in the li…

astro-ph.SR2021

Transport coefficients enhanced by suprathermal particles in nonequilibrium heliospheric plasmas

Edin Husidic, Marian Lazar, Horst Fichtner +2

In heliospheric plasmas the transport of energy and particles is governed by various fluxes (e.g., heat flux) triggered by different forces, electromagnetic fields, and gradients i…

physics.plasm-ph2021★ 15 cited

A new low-beta regime for unstable proton firehose modes in bi-Kappa distributed plasmas

S. M. Shaaban, M. Lazar, R. F. Wimmer-Schweingruber +1

In the solar wind plasma an excess of kinetic temperature along the background magnetic field stimulates proton firehose modes to grow if the parallel plasma beta parameter is suff…

astro-ph.SR2020★ 12 cited

Generalized anisotropic -cookbook: 2D fitting of Ulysses electron data

Klaus Scherer, Edin Husidic, Marian Lazar +1

Observations in space plasmas reveal particle velocity distributions out of thermal equilibrium, with anisotropies (e.g., parallel drifts or/and different temperatures, $T_\paralle…

physics.space-ph2020★ 17 cited

On the Generation of Compressible Mirror-mode Fluctuations in the Inner Heliosheath

Horst Fichtner, Jens Kleimann, Peter H. Yoon +3

Measurements made with the Voyager 1 spacecraft indicate that significant levels of compressive fluctuations exist in the inner heliosheath. Some studies have already been performe…

astro-ph.SR2020★ 21 cited

The -cookbook: a novel generalizing approach to unify -like distributions for plasma particle modeling

Klaus Scherer, Edin Husidic, Marian Lazar +1

In the literature different so-called -distribution functions are discussed to fit and model the velocity (or energy) distributions of solar wind species, pickup ions or magneto…

astro-ph.SR2020★ 36 cited

On the Diversity of M-Star Astrospheres and the Role of Galactic Cosmic Rays Within

Konstantin Herbst, Klaus Scherer, Stefan E. S. Ferreira +7

With upcoming missions such as the James Webb Space Telescope (JWST), the European Extremely Large Telescope (ELT), and the Atmospheric Remote-sensing Infrared Exoplanet Large-surv…

physics.plasm-ph2020★ 24 cited

Linear Dispersion Theory of Parallel Electromagnetic Modes for Regularized Kappa-Distributions

Edin Husidic, Marian Lazar, Horst Fichtner +2

The velocity particle distributions measured in-situ in space plasmas deviate from Maxwellian (thermal) equilibrium, showing enhanced suprathermal tails which are well described by…

astro-ph.SR2020★ 8 cited

A new class of discontinuous solar wind solutions

Bidzina M. Shergelashvili, Velentin N. Melnik, Grigol Dididze +6

A new class of one-dimensional solar wind models is developed within the general polytropic, single-fluid hydrodynamic framework. The particular case of quasi-adiabatic radial expa…

astro-ph.SR2020★ 34 cited

MHD-shock structures of astrospheres: Cephei-like astrospheres

K. Scherer, L. R. Baalmann, H. Fichtner +5

The interpretation of recent observations of bow shocks around O-stars and the creation of corresponding models require a detailed understanding of the associated (magneto-)hydrody…

astro-ph.SR2020★ 15 cited

Skymaps of observables of three-dimensional MHD astrosphere models

L. R. Baalmann, K. Scherer, H. Fichtner +3

Three-dimensional models of astrospheres have recently become of interest. However, comparisons between these models and observations are non-trivial because of the two-dimensional…

astro-ph.SR2019★ 6 cited

An empirical model of Energetic Neutral Atom imaging of the heliosphere and its implications for future heliospheric missions at great heliocentric distances

Andre Galli, Peter Wurz, Horst Fichtner +2

Several concepts for heliospheric missions operating at heliocentric distances far beyond Earth orbit are currently investigated by the scientific community. The mission concept of…

physics.space-ph2019★ 26 cited

Whistler instability stimulated by the suprathermal electrons present in space plasmas

M. Lazar, R. A. Lopez, S. M. Shaaban +2

In the absence of efficient collisions, deviations from thermal equilibrium of plasma particle distributions are controlled by the self-generated instabilities. The whistler instab…

physics.comp-ph2019★ 43 cited

Moments of the anisotropic regularized -distributions

Klaus Scherer, Marian Lazar, Edin Husidic +1

For collisionless (or collision-poor) plasma populations which are well described by the -distribution functions (also known as the Kappa or Lorentzian power-laws) a macroscopic…

physics.plasm-ph2019★ 33 cited

On the applicability of -distributions

Klaus Scherer, Horst Fichtner, Hans-Jörg Fahr +1

The standard (non-relativistic) -distribution is widely used to fit data and to describe macroscopic thermodynamical behavior, e.g.\ the pressure (temperature) as the second mom…