Scaling laws for the energy transfer in space plasma turbulence

R Marino, L Sorriso-Valvo - Physics Reports, 2023 - Elsevier
One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …

Solar wind electrons alphas and protons (SWEAP) investigation: Design of the solar wind and coronal plasma instrument suite for solar probe plus

JC Kasper, R Abiad, G Austin, M Balat-Pichelin… - Space Science …, 2016 - Springer
Abstract The Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Solar
Probe Plus is a four sensor instrument suite that provides complete measurements of the …

Theory and transport of nearly incompressible magnetohydrodynamic turbulence

GP Zank, L Adhikari, P Hunana, D Shiota… - The Astrophysical …, 2017 - iopscience.iop.org
The theory of nearly incompressible magnetohydrodynamics (NI MHD) was developed
largely in the early 1990s, together with an important extension to inhomogeneous flows in …

Shear-driven transition to isotropically turbulent solar wind outside the Alfvén critical zone

D Ruffolo, WH Matthaeus, R Chhiber… - The Astrophysical …, 2020 - iopscience.iop.org
Shear-driven Transition to Isotropically Turbulent Solar Wind Outside the Alfvén Critical Zone -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of …

The solar wind as a turbulence laboratory

R Bruno, V Carbone - Living Reviews in Solar Physics, 2013 - Springer
In this review we will focus on a topic of fundamental importance for both astrophysics and
plasma physics, namely the occurrence of large-amplitude low-frequency fluctuations of the …

The ACE magnetic fields experiment

CW Smith, J L'Heureux, NF Ness, MH Acuna… - The advanced …, 1998 - Springer
The magnetic field experiment on ACE provides continuous measurements of the local
magnetic field in the interplanetary medium. These measurements are essential in the …

Observational constraints on the dynamics of the interplanetary magnetic field dissipation range

RJ Leamon, CW Smith, NF Ness… - Journal of …, 1998 - Wiley Online Library
The dissipation range for interplanetary magnetic field fluctuations is formed by those
fluctuations with spatial scales comparable to the gyroradius or ion inertial length of a …

Coherent structures, intermittent turbulence, and dissipation in high-temperature plasmas

H Karimabadi, V Roytershteyn, M Wan… - Physics of …, 2013 - pubs.aip.org
An unsolved problem in plasma turbulence is how energy is dissipated at small scales.
Particle collisions are too infrequent in hot plasmas to provide the necessary dissipation …

Interaction of the solar wind with the local interstellar medium: A theoretical perspective

GP Zank - Space Science Reviews, 1999 - Springer
The interaction of the solar wind with the local interstellar medium (LISM) is attracting
renewed interest, thanks to the possibility that the Voyager spacecraft may, in the not too …

Secondary antiprotons and propagation of cosmic rays in the galaxy and heliosphere

IV Moskalenko, AW Strong, JF Ormes… - The Astrophysical …, 2002 - iopscience.iop.org
High-energy collisions of cosmic-ray nuclei with interstellar gas are believed to be the
mechanism producing the majority of cosmic-ray antiprotons. Because of the kinematics of …