Theory of cosmic ray transport in the heliosphere
Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global
challenge in the field of heliophysics, in that such a study, if it were to be performed from first …
challenge in the field of heliophysics, in that such a study, if it were to be performed from first …
Mesoscale structure in the solar wind
NM Viall, CE DeForest, L Kepko - Frontiers in Astronomy and Space …, 2021 - frontiersin.org
Structures in the solar wind result from two basic mechanisms: structures injected or
imposed directly by the Sun, and structures formed through processing en route as the solar …
imposed directly by the Sun, and structures formed through processing en route as the solar …
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 …
On the transmission of turbulent structures across the earth's bow shock
Collisionless shocks and plasma turbulence are crucial ingredients for a broad range of
astrophysical systems. The shock–turbulence interaction, and in particular the transmission …
astrophysical systems. The shock–turbulence interaction, and in particular the transmission …
Relativistic particle transport and acceleration in structured plasma turbulence
We discuss the phenomenon of energization of relativistic charged particles in three-
dimensional incompressible MHD turbulence and the diffusive properties of the motion of …
dimensional incompressible MHD turbulence and the diffusive properties of the motion of …
[HTML][HTML] Predictability of variable solar–terrestrial coupling
Abstract In October 2017, the Scientific Committee on Solar-Terrestrial Physics (SCOSTEP)
Bureau established a committee for the design of SCOSTEP's Next Scientific Programme …
Bureau established a committee for the design of SCOSTEP's Next Scientific Programme …
The S-Web Origin of Composition Enhancement in the Slow-to-moderate Speed Solar Wind
BJ Lynch, NM Viall, AK Higginson, L Zhao… - The Astrophysical …, 2023 - iopscience.iop.org
Connecting the solar wind observed throughout the heliosphere to its origins in the solar
corona is one of the central aims of heliophysics. The variability in the magnetic field, bulk …
corona is one of the central aims of heliophysics. The variability in the magnetic field, bulk …
On the turbulent reduction of drifts for solar energetic particles
JP Van den Berg, NE Engelbrecht… - The Astrophysical …, 2021 - iopscience.iop.org
Particle drifts perpendicular to the background magnetic field have been proposed by some
authors as an explanation for the very efficient perpendicular transport of solar energetic …
authors as an explanation for the very efficient perpendicular transport of solar energetic …
Magnetic reconnection as a mechanism to produce multiple thermal proton populations and beams locally in the solar wind
B Lavraud, R Kieokaew, N Fargette, P Louarn… - Astronomy & …, 2021 - aanda.org
Context. Spacecraft data revealed early on the frequent observation of multiple near-thermal
proton populations in the solar wind. Decades of research on their origin have focused on …
proton populations in the solar wind. Decades of research on their origin have focused on …
Modelling two energetic storm particle events observed by Solar Orbiter using the combined EUHFORIA and iPATH models
Context. By coupling the EUropean Heliospheric FORcasting Information Asset (EUHFORIA)
and the improved Particle Acceleration and Transport in the Heliosphere (iPATH) models …
and the improved Particle Acceleration and Transport in the Heliosphere (iPATH) models …