collaborators

9 papers

astro-ph.SR2026

Evidence of global periodicity in PSP data: can they be linked to long-period oscillations in solar active regions?

G. Dumbadze, B. M. Shergelashvili, M. Khodachenko +4

The presence of coherent oscillatory signatures in Parker Solar Probe SWEAP datasets, identified through a series of spectral analyses, is addressed, and their possible connection…

physics.plasm-ph2026

Wave instabilities in anisotropic regularized Kappa plasmas: New plasma dispersion functions and numerical validation

Rudi Gaelzer, Dustin L. Schröder, Marian Lazar +1

Plasmas in space and astrophysical environments are frequently found in (quasi-)stationary states not in thermal equilibrium, indicated by velocity distribution functions (VDFs) fe…

physics.plasm-ph2026

Hybrid simulations of the proton beam instabilities in the young solar wind. The formation of hammerhead-like distributions

R. A. López, Shaaban M. Shaaban, M. Lazar +4

Parker Solar Probe (PSP) observations in the young solar wind reveal new properties of both plasma particle velocity distributions (VDs) and associated electromagnetic (EM) wave fl…

astro-ph.SR2026

Polytropic stellar wind models with strongly localized heating

L. Westrich, B. Shergelashvili, H. Fichtner +1

Polytropic models of stellar winds remain to be useful tools because they allow for a simple description of the energy balance of the expanding plasma without explicitly specifying…

physics.plasm-ph2026

Modeling complex plasma instabilities in space plasmas - Three-component electron formalism of heat-flux instabilities

Dustin L. Schröder, Marian Lazar, Horst Fichtner +2

Despite the fact that electrons observed in situ in space plasmas have three major components-the quasi-thermal core, suprathermal halo, and strahl-the analysis of instabilities tr…

astro-ph.HE2026

The impact of Solar magnetic field configurations on the production of gamma rays at the Solar disk

Julien Dörner, Frederic Effenberger, Horst Fichtner +4

The Sun produces a steady signal of high-energy gamma rays through interactions of Galactic cosmic rays (GCRs) with its atmosphere. Observations with Fermi-LAT and HAWC have reveal…