[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 …
Linear Mode Decomposition in Magnetohydrodynamics Revisited
GP Zank, LL Zhao, L Adhikari… - The Astrophysical …, 2023 - iopscience.iop.org
Small-amplitude fluctuations in the magnetized solar wind are measured typically by a
single spacecraft. In the magnetohydrodynamics (MHD) description, fluctuations are typically …
single spacecraft. In the magnetohydrodynamics (MHD) description, fluctuations are typically …
Current sheets, plasmoids and flux ropes in the heliosphere: Part ii: Theoretical aspects
Our understanding of processes occurring in the heliosphere historically began with
reduced dimensionality-one-dimensional (1D) and two-dimensional (2D) sketches and …
reduced dimensionality-one-dimensional (1D) and two-dimensional (2D) sketches and …
Flux ropes, turbulence, and collisionless perpendicular shock waves: High plasma beta case
With the onset of solar maximum and the expected increased prevalence of interplanetary
shock waves, Parker Solar Probe is likely to observe numerous shocks in the next few years …
shock waves, Parker Solar Probe is likely to observe numerous shocks in the next few years …
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 …
Solar wind turbulence: connections with energetic particles
S Oughton, NE Engelbrecht - New Astronomy, 2021 - Elsevier
For the solar wind, a wealth of observational evidence indicates that turbulence is an
important dynamical process for velocity (v), magnetic (b), and other related fluctuations at …
important dynamical process for velocity (v), magnetic (b), and other related fluctuations at …
Identification of coherent structures in space plasmas: the magnetic helicity–PVI method
Context. Plasma turbulence can be viewed as a magnetic landscape populated by large-
and small-scale coherent structures. In this complex network, large helical magnetic tubes …
and small-scale coherent structures. In this complex network, large helical magnetic tubes …
Parker Solar Probe observations of helical structures as boundaries for energetic particles
Energetic particle transport in the interplanetary medium is known to be affected by magnetic
structures. It has been demonstrated for solar energetic particles in near-Earth orbit studies …
structures. It has been demonstrated for solar energetic particles in near-Earth orbit studies …
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 …
Modeling energetic particle acceleration and transport in a solar wind region with contracting and reconnecting small-scale flux ropes at Earth orbit
JA Le Roux, GM Webb, OV Khabarova… - The Astrophysical …, 2019 - iopscience.iop.org
New analytical steady-state and time-dependent solutions for the acceleration of energetic
particles by contracting and reconnecting small-scale flux ropes (SMFRs) in the solar wind …
particles by contracting and reconnecting small-scale flux ropes (SMFRs) in the solar wind …