This Letter provides a concrete implementation of Fermi's model of particle acceleration in
magnetohydrodynamic (MHD) turbulence, connecting the rate of energization to the …

Magnetic fields are a dynamically important component of the turbulent interstellar medium
(ISM) of star-forming galaxies. These magnetic fields are due to a dynamo action, which is a …

Particle transport through localized interactions with sharp magnetic field bends in MHD
turbulence Page 1 J. Plasma Phys. (2023), vol. 89, 175890501 © The Author(s), 2023 …

In star-forming galaxies, the far-infrared (FIR) and radio-continuum luminosities obey a tight
empirical relation over a large range of star-formation rates (SFR). To understand the …

Nonthermal acceleration of particles in magnetohydrodynamic (MHD) turbulence plays a
central role in a wide variety of astrophysical sites. This physics is addressed here in the …

In weakly collisional and collisionless magnetized plasmas, the pressure–strain interaction
describes the rate of conversion between bulk flow and thermal energy density. In this study …

Context. Prominences are cool, dense clouds suspended within the solar corona. Their in
situ formation through the levitation-condensation mechanism is a textbook example of the …

The warm–hot intergalactic medium (warm–hot IGM, or WHIM) pervades the filaments of the
Cosmic Web and harbours half of the Universe's baryons. The WHIM's thermodynamic …

Magnetic field lines in interstellar media have a rich morphology, which could be
characterized by geometrical parameters such as curvature and torsion. In this paper we …

Context. Magnetic switchbacks are magnetic structures characterized as intervals of sudden
reversal in the radial component of the pristine solar wind's magnetic field. Switchbacks …