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 …
Solar wind turbulence and the role of ion instabilities
Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In
addition to the presence of magnetic field, the differences with neutral fluid isotropic …
addition to the presence of magnetic field, the differences with neutral fluid isotropic …
Astrophysical gyrokinetics: kinetic and fluid turbulent cascades in magnetized weakly collisional plasmas
This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …
astrophysical plasmas. It is motivated by observations of electromagnetic and density …
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 …
Anisotropic scaling of magnetohydrodynamic turbulence
TS Horbury, M Forman, S Oughton - Physical Review Letters, 2008 - APS
We present a quantitative estimate of the anisotropic power and scaling of magnetic field
fluctuations in inertial range magnetohydrodynamic turbulence, using a novel wavelet …
fluctuations in inertial range magnetohydrodynamic turbulence, using a novel wavelet …
The evolution and role of solar wind turbulence in the inner heliosphere
The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - IOPscience This
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site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
Dissipation and heating in solar wind turbulence: from the macro to the micro and back again
The past decade has seen a flurry of research activity focused on discerning the physics of
kinetic scale turbulence in high-speed astrophysical plasma flows. By 'kinetic'we mean …
kinetic scale turbulence in high-speed astrophysical plasma flows. By 'kinetic'we mean …
Geoeffectiveness of interplanetary Alfvén waves. I. Magnetopause magnetic reconnection and directly driven substorms
L Dai, Y Han, C Wang, S Yao, W Gonzalez… - The Astrophysical …, 2023 - iopscience.iop.org
In particular during the descending phase of the solar cycle, Alfvén waves in the high-speed
solar wind streams are a major form of interplanetary disturbances. The fluctuating …
solar wind streams are a major form of interplanetary disturbances. The fluctuating …
Mesoscale structure in the solar wind
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 …
Anisotropy of Alfvénic turbulence in the solar wind and numerical simulations
We investigate the anisotropy of Alfvénic turbulence in the inertial range of slow solar wind
and in both driven and decaying reduced magnetohydrodynamic simulations. A direct …
and in both driven and decaying reduced magnetohydrodynamic simulations. A direct …