HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division
designed to explore the dynamic three-dimensional mechanisms controlling the physics of …

The nature of cosmic ray (CR) transport in the Milky Way remains elusive. The predictions of
current microphysical CR transport models in magnetohydrodynamic (MHD) turbulence are …

We investigate the spectral properties of the electromagnetic fluctuations of sub-ion scale
turbulence in weakly collisional, low-beta plasmas using a two-field isothermal gyrofluid …

Active processes drive biological dynamics across various scales and include subcellular
cytoskeletal remodelling, tissue development in embryogenesis and the population-level …

The processes controlling the complex clump structure, phase distribution, and magnetic
field geometry that develop across a broad range of scales in the turbulent interstellar …

Turbulence plays a key role in forming the complex geometry of the large-scale current
sheet (CS) and fast energy release in a solar eruption. In this paper, we present full 3D high …

Magnetic reconnection within a highly magnetized plasma has been seen as a viable
mechanism to extract the energy from a rotating black hole, as it can generate negative …

Solar flares can release coronal magnetic energy explosively and may impact the safety of
near-Earth space environments. Their structures and properties on the macroscale have …

We analyze a merged Parker Solar Probe (PSP) and Solar Orbiter (SO) data set covering
heliocentric distances 13 R⊙≲ R≲ 220 R⊙ to investigate the radial evolution of power and …

To comprehensively understand the saturation of two-dimensional (2D) magnetized Kelvin–
Helmholtz-instability-driven turbulence, energy transfer analysis is extended from the …