SFB1491 - Cosmic Interacting Matters
|
Title |
Citation |
Project(s) |
SFB Authors (alphabetical order) |
|---|---|---|---|
| Clustering Wind data at 1 AU to contextualize magnetic reconnection in the solar wind | [Carella et al., 2025, A&A , 701 , A212] | F2 | |
| Energetic spectra from semi-implicit particle-in-cell simulations of magnetic reconnection | [Schoeffler et al., 2025, arXiv e-prints , arXiv:2509.11100] | F2 | |
| Impact of nonthermal electron distributions on the triggering of the ion-ion acoustic instability near the Sun: Kinetic simulations | [Afify et al., 2025, arXiv e-prints , arXiv:2509.18032] | F2 | |
| Optimal Landau-type closure parameters for two-fluid simulations of plasma turbulence at kinetic scales | [Lautenbach et al., 2025, accepted and to appear in J. Plasma Physics. , arXiv:2509.08525] | F1, F2, F7 | |
| Anisotropic heating and parallel heat flux in electron-only magnetic reconnection with intense guide fields | [Ren et al., 2025, Journal of Plasma Physics , 91.4 , E105] | F2 | |
| Can plasma physics establish a significant bound on long-range dark matter interactions? | [Schoeffler et al., 2025, Phys. Rev. D , 111 , L071701] | F2, F5, F6 | |
| Particle-in-cell simulations of the tearing instability for relativistic pair plasmas | [Schoeffler et al., 2025, Journal of Plasma Physics , 91.1 , E42] | A5, F2 | |
| Quasi-parallel Antisunward-propagating Whistler Waves Associated with the Electron Deficit in the Near-Sun Solar Wind: Particle-in-cell Simulation | [Micera et al., 2025, The Astrophysical Journal , 979.2 , 226] | F2 | |
| Fully Kinetic Simulations of Proton-beam-driven Instabilities from Parker Solar Probe Observations | [Pezzini et al., 2024, The Astrophysical Journal , 975.1 , 37] | F2 | |
| Nonlocal contributions to the turbulent cascade in magnetohydrodynamic plasmas | [Friedrich et al., 2024, Phys. Rev. E , 109 , 045208] | F1, F2 | |
| The Regulation of the Solar Wind Electron Heat Flux by Wave–Particle Interactions | [Coburn et al., 2024, ApJ , 964.1 , 100] | F2 | |
| Applications of Fast Magnetic Reconnection Models to the Atmospheres of the Sun and Protoplanetary Disks | [Pucci et al., 2024, The Astrophysical Journal , 970.1 , 87] | F2 | |
| Clustering of global magnetospheric observations | [Edmond et al., 2024, Journal of Geophysical Research: Machine Learning and Computation , 1.4 , e2024JH000221] | F2 | |
| Electrostatic Bursts Generated by the Ion–Ion Acoustic Instability with Solar Wind Plasma Parameters | [Afify et al., 2024, The Astrophysical Journal , 971.1 , 93] | F2 | |
| The muphyII code: Multiphysics plasma simulation on large HPC systems | [Allmann-Rahn et al., 2024, Computer Physics Communications , 296 , 109064] | F2 | |
| Generation of Subion Scale Magnetic Holes from Electron Shear Flow Instabilities in Plasma Turbulence | [Arrò et al., 2023, The Astrophysical Journal , 958.1 , 11] | F2 | |
| Energy Conversion by Magnetic Reconnection in Multiple Ion Temperature Plasmas | [Dargent et al., 2023, Geophys. Res. Lett. , 50.12 , e2023GL103324] | F2 | |
| High-energy synchrotron flares powered by strongly radiative relativistic magnetic reconnection: 2D and 3D PIC simulations | [Schoeffler et al., 2023, Monthly Notices of the Royal Astronomical Society , 523.3 , 3812-3839] | F2 | |
| Unsupervised classification of fully kinetic simulations of plasmoid instability using self-organizing maps (SOMs) | [Köhne et al., 2023, Journal of Plasma Physics , 89.3 , 895890301] | F2 | |
| Particle-in-cell simulations of Alfvén wave parametric decay in a low-beta plasma | [González et al., 2023, Journal of Plasma Physics , 89.2 , 905890208] | F2 | |
| Using Unsupervised Machine Learning to make new discoveries in space data | [Lapenta et al., 2023, Artificial Intelligence for Space: AI4SPACE: Trends, Applications, and Perspectives , 214] | F2 | |
| Electron-Driven Instabilities in the Solar Wind | [Verscharen et al., 2022, Frontiers in Astronomy and Space Sciences , 9 , 951628] | F2 | |
| Interaction between electrostatic collisionless shocks generates strong magnetic fields | [Boella et al., 2022, New Journal of Physics , 24.6 , 063016] | F2 |