output
20042026
most citedExploring the Sensitivity of Next Generation Gravitational Wave Detectors

1.2k citations

56 papers

physics.space-ph2026

High-energy Particle Transport in Three-dimensional Anisotropic Turbulent Magnetic Fields

Daniela Maci, Rony Keppens, Fabio Bacchini

The understanding and modeling of high-energy particles transport in turbulent magnetic fields is an important open question in space- and astrophysics. The multiscale, nonlinear n…

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

Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter

Xiaohang Chen, Gang Li, Joe Giacalone +12

The propagation of solar energetic particles (SEPs) through the heliosphere is primarily guided by the interplanetary magnetic field (IMF) which is embedded in the solar wind plasm…

astro-ph.SR2026

Chromosphere of the quiet sun: II. Atmospheric response to small-scale magnetic flux emergence

Quentin Noraz, Mats Carlsson, Guillaume Aulanier

Coupling between the photosphere, chromosphere and corona in the quiet Sun (QS) is governed by a complex interplay between magnetic structuring, heating, mass loading, and radiativ…

astro-ph.SR2026

Thermal instability in coronal loops: linking eigenvalue spectra to time-dependent evolution

Adrian Kelly, Rony Keppens, Jordi De Jonghe

Cool, dense condensations such as coronal rain and prominences suggest that coronal plasma can undergo runaway radiative cooling. Connecting this behaviour to linear thermal modes…

astro-ph.IM2026

Thermal background reduction for mid-infrared imaging by low-rank background and sparse point-source modelling

R. A. R. Moens, A. G. M. Pietrow, B. Brandl +1

Mid-infrared astronomy from the ground faces critical challenges in accurately detecting and quantifying sources due to the dominant spatially and time-variable background noise. M…