activity
20192026
most citedMoments of the anisotropic regularized -distributions

43 citations · 119 across the 12 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2026

Wave-Growth-Limited Particle Confinement in a Near-Parallel Interplanetary Shock Observed by Parker Solar Probe

A. Kouloumvakos, I. C. Jebaraj, M. A. Malkov +11

Collisionless shocks confine the particles they accelerate with the upstream wave field they themselves drive. Streaming particles resonantly amplify Alfvén waves, and the waves th…

astro-ph.SR2026

Does Diffusive Shock Acceleration Reach Steady State? Insights from a Near-Sun Shock Observed by Parker Solar Probe

Immanuel Christopher Jebaraj, Mikhail Malkov, Nicolas Wijsen +7

Collisionless shocks accelerate particles at a rate set by the diffusion coefficient of those particles in waves they themselves generate. Theory fixes that coefficient only in ste…

astro-ph.SR2026

The Wave-Regulated Precursor of a Near-Parallel Interplanetary Shock Observed by Parker Solar Probe

Immanuel Christopher Jebaraj, Lucas Colomban, Oleksiy Agapitov +7

Diffusive shock acceleration, at shocks from coronal mass ejections to supernova-remnant blast waves, presupposes a scattering wave field that the accelerated particles themselves…

astro-ph.SR2025

COCONUT: A coronal model with an energy decomposition strategy

Haopeng Wang, Stefaan Poedts, Andrea Lani +11

In this paper, we propose an energy decomposition method combined with an HLL Riemann solver that includes an additional dissipation term in the energy equation to improve the nume…

astro-ph.SR2025★ 1 cited

Modelling gyrosynchrotron emission from coronal energetic electrons in a CME flux rope

Edin Husidic, Nicolas Wijsen, Immanuel Christopher Jebaraj +4

Solar flares and coronal mass ejections (CMEs) can accelerate electrons, causing bursts such as type IV emissions in the solar radio continuum. Although radio spectroscopy is a pow…

astro-ph.SR2025

SIP-IFVM: A time-evolving coronal model with an extended magnetic field decomposition strategy

Haopeng Wang, Liping Yang, Stefaan Poedts +20

Time-evolving magnetohydrodynamic (MHD) coronal modeling, driven by a series of time-dependent photospheric magnetograms, represents a new generation of coronal simulations. This a…