Solar modulation of cosmic rays
MS Potgieter - Living Reviews in Solar Physics, 2013 - Springer
This is an overview of the solar modulation of cosmic rays in the heliosphere. It is a broad
topic with numerous intriguing aspects so that a research framework has to be chosen to …
topic with numerous intriguing aspects so that a research framework has to be chosen to …
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 …
[HTML][HTML] 3D turbulent reconnection: Theory, tests, and astrophysical implications
Magnetic reconnection, topological changes in magnetic fields, is a fundamental process in
magnetized plasmas. It is associated with energy release in regions of magnetic field …
magnetized plasmas. It is associated with energy release in regions of magnetic field …
Particle acceleration in relativistic plasma turbulence
Due to its ubiquitous presence, turbulence is often invoked to explain the origin of
nonthermal particles in astrophysical sources of high-energy emission. With particle-in-cell …
nonthermal particles in astrophysical sources of high-energy emission. With particle-in-cell …
The interplay of magnetically dominated turbulence and magnetic reconnection in producing nonthermal particles
Magnetized turbulence and magnetic reconnection are often invoked to explain the
nonthermal emission observed from a wide variety of astrophysical sources. By means of …
nonthermal emission observed from a wide variety of astrophysical sources. By means of …
Fast particle acceleration in three-dimensional relativistic reconnection
Magnetic reconnection is invoked as one of the primary mechanisms to produce energetic
particles. We employ large-scale 3D particle-in-cell simulations of reconnection in …
particles. We employ large-scale 3D particle-in-cell simulations of reconnection in …
Ion and electron acceleration in fully kinetic plasma turbulence
Turbulence is often invoked to explain the origin of nonthermal particles in space and
astrophysical plasmas. By means of 3D fully kinetic particle-in-cell simulations, we …
astrophysical plasmas. By means of 3D fully kinetic particle-in-cell simulations, we …
Hidden cores of active galactic nuclei as the origin of medium-energy neutrinos: critical tests with the MeV gamma-ray connection
Mysteries about the origin of high-energy cosmic neutrinos have deepened by the recent
IceCube measurement of a large diffuse flux in the 10–100 TeV range. Based on the …
IceCube measurement of a large diffuse flux in the 10–100 TeV range. Based on the …
The origin of underdense plasma downflows associated with magnetic reconnection in solar flares
Magnetic reconnection is a universal process that powers explosive energy-release events
such as solar flares, geomagnetic substorms and some astrophysical jets. A characteristic …
such as solar flares, geomagnetic substorms and some astrophysical jets. A characteristic …
Three-dimensional modelling of the shock–turbulence interaction
The complex interaction between shocks and plasma turbulence is extremely important to
address crucial features of energy conversion in a broad range of astrophysical systems. We …
address crucial features of energy conversion in a broad range of astrophysical systems. We …