The multi-scale nature of the solar wind
D Verscharen, KG Klein, BA Maruca - Living Reviews in Solar Physics, 2019 - Springer
The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …
associated with its characteristic spatial and temporal scales. The characteristic length …
Magnetic field amplification in galaxy clusters and its simulation
J Donnert, F Vazza, M Brüggen, J ZuHone - Space Science Reviews, 2018 - Springer
We review the present theoretical and numerical understanding of magnetic field
amplification in cosmic large-scale structure, on length scales of galaxy clusters and beyond …
amplification in cosmic large-scale structure, on length scales of galaxy clusters and beyond …
But what about...: cosmic rays, magnetic fields, conduction, and viscosity in galaxy formation
PF Hopkins, TK Chan… - Monthly Notices of …, 2020 - academic.oup.com
We present and study a large suite of high-resolution cosmological zoom-in simulations,
using the FIRE-2 treatment of mechanical and radiative feedback from massive stars …
using the FIRE-2 treatment of mechanical and radiative feedback from massive stars …
Dynamo theories
F Rincon - Journal of Plasma Physics, 2019 - cambridge.org
These lecture notes are based on a tutorial given in 2017 at a plasma physics winter school
in Les Houches. Their aim is to provide a self-contained graduate-student level introduction …
in Les Houches. Their aim is to provide a self-contained graduate-student level introduction …
A characteristic scale for cold gas
M McCourt, SP Oh, R O'Leary… - Monthly Notices of the …, 2018 - academic.oup.com
We find that clouds of optically thin, pressure-confined gas are prone to fragmentation as
they cool below∼ 106 K. This fragmentation follows the lengthscale∼ cst cool, ultimately …
they cool below∼ 106 K. This fragmentation follows the lengthscale∼ cst cool, ultimately …
Kinetic Turbulence in Collisionless High- Plasmas
We present results from three-dimensional hybrid-kinetic simulations of Alfvénic turbulence
in a high-β, collisionless plasma. The key feature of such turbulence is the interplay between …
in a high-β, collisionless plasma. The key feature of such turbulence is the interplay between …
A universal power-law prescription for variability from synthetic images of black hole accretion flows
The Event Horizon Telescope (EHT) has opened a new window on supermassive black
holes. With the advent of millimeter and submillimeter very long baseline interferometry …
holes. With the advent of millimeter and submillimeter very long baseline interferometry …
A new bound on axion-like particles
MCD Marsh, HR Russell, AC Fabian… - … of Cosmology and …, 2017 - iopscience.iop.org
Axion-like particles (ALPs) and photons can quantum mechanically interconvert when
propagating through magnetic fields, and ALP-photon conversion may induce oscillatory …
propagating through magnetic fields, and ALP-photon conversion may induce oscillatory …
[HTML][HTML] The basis for cosmic ray feedback: Written on the wind
EG Zweibel - Physics of Plasmas, 2017 - pubs.aip.org
Star formation and supermassive black hole growth in galaxies appear to be self-limiting.
The mechanisms for self-regulation are known as feedback. Cosmic rays, the relativistic …
The mechanisms for self-regulation are known as feedback. Cosmic rays, the relativistic …
First Sagittarius A* Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring
In a companion paper, we present the first spatially resolved polarized image of Sagittarius
A* on event horizon scales, captured using the Event Horizon Telescope, a global very long …
A* on event horizon scales, captured using the Event Horizon Telescope, a global very long …