[HTML][HTML] Turbulence in the outer heliosphere
The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their
interaction is governed by complex physical processes and creates heliospheric regions …
interaction is governed by complex physical processes and creates heliospheric regions …
[HTML][HTML] HelioSwarm: a multipoint, multiscale mission to characterize turbulence
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 …
designed to explore the dynamic three-dimensional mechanisms controlling the physics of …
Nine outstanding questions of solar wind physics
NM Viall, JE Borovsky - Journal of Geophysical Research …, 2020 - Wiley Online Library
In situ measurements of the solar wind have been available for almost 60 years, and in that
time plasma physics simulation capabilities have commenced and ground‐based solar …
time plasma physics simulation capabilities have commenced and ground‐based solar …
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 …
Solar wind turbulence from 1 to 45 au. IV. Turbulent transport and heating of the solar wind using Voyager observations
We adopt the theory for turbulent transport of energy by solar wind fluctuations and apply
that theory to observations by the Voyager 1 and 2 spacecraft to obtain rates of thermal …
that theory to observations by the Voyager 1 and 2 spacecraft to obtain rates of thermal …
Towards a deeper understanding of historic cosmic ray modulation during solar cycle 20
NE Engelbrecht, CP Wolmarans - Advances in Space Research, 2020 - Elsevier
Given recent successes in modelling the transport of cosmic rays (CRs) in the heliosphere
from first principles, taking into account the behaviour of heliospheric turbulence quantities …
from first principles, taking into account the behaviour of heliospheric turbulence quantities …
[HTML][HTML] Driving and Dissipation of Solar-Wind Turbulence: What is the Evidence?
CW Smith, BJ Vasquez - Frontiers in Astronomy and Space Sciences, 2021 - frontiersin.org
Fifty years of solar wind observations have provided extensive data that drives an evolving
view of the fundamental nature and dynamics of the magnetic, velocity, and density …
view of the fundamental nature and dynamics of the magnetic, velocity, and density …
Spectral transfer and Kármán–Howarth–Monin equations for compressible hall magnetohydrodynamics
We derive two new forms of the Kármán–Howarth–Monin (KHM) equation for decaying
compressible Hall magnetohydrodynamic (MHD) turbulence. We test them on results of a …
compressible Hall magnetohydrodynamic (MHD) turbulence. We test them on results of a …
Lagrangian Perspectives on the Small-scale Structure of Alfvénic Turbulence and Stochastic Models for the Dispersion of Fluid Particles and Magnetic Field Lines in …
NH Bian, G Li - The Astrophysical Journal Supplement Series, 2024 - iopscience.iop.org
Lagrangian perspectives on the small-scale structure of anisotropic Alfvénic turbulence are
adopted. We are interested in relating the statistical properties of the Eulerian field …
adopted. We are interested in relating the statistical properties of the Eulerian field …
Magnetic waves excited by newborn interstellar pickup ions measured by the Voyager spacecraft from 1 to 45 au. II. Instability and turbulence analyses
In this companion paper, we describe low-frequency magnetic waves observed in 637
intervals of Voyager 1 and 2 data from launch late in 1977 through 1990. By the end of 1990 …
intervals of Voyager 1 and 2 data from launch late in 1977 through 1990. By the end of 1990 …