Scaling laws for the energy transfer in space plasma turbulence
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 …
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
Recent progress in astrophysical plasma turbulence from solar wind observations
CHK Chen - Journal of Plasma Physics, 2016 - cambridge.org
This paper summarises some of the recent progress that has been made in understanding
astrophysical plasma turbulence in the solar wind, from in situ spacecraft observations. At …
astrophysical plasma turbulence in the solar wind, from in situ spacecraft observations. At …
[HTML][HTML] The solar orbiter mission-science overview
D Müller, OCS Cyr, I Zouganelis, HR Gilbert… - Astronomy & …, 2020 - aanda.org
Aims. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015–2025 programme and a
mission of international collaboration between ESA and NASA, will explore the Sun and …
mission of international collaboration between ESA and NASA, will explore the Sun and …
First in situ measurements of electron density and temperature from quasi-thermal noise spectroscopy with Parker Solar Probe/FIELDS
Heat transport in the solar corona and wind is still a major unsolved astrophysical problem.
Because of the key role played by electrons, the electron density and temperature (s) are …
Because of the key role played by electrons, the electron density and temperature (s) are …
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
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
Intermittency, nonlinear dynamics and dissipation in the solar wind and astrophysical plasmas
An overview is given of important properties of spatial and temporal intermittency, including
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …
Ion‐scale spectral break of solar wind turbulence at high and low beta
The power spectrum of magnetic fluctuations in the solar wind at 1 AU displays a break
between two power laws in the range of spacecraft‐frame frequencies 0.1 to 1 Hz. These …
between two power laws in the range of spacecraft‐frame frequencies 0.1 to 1 Hz. These …
In Situ Signature of Cyclotron Resonant Heating in the Solar Wind
The dissipation of magnetized turbulence is an important paradigm for describing heating
and energy transfer in astrophysical environments such as the solar corona and wind; …
and energy transfer in astrophysical environments such as the solar corona and wind; …
A kinetic model of plasma turbulence
A Hybrid Vlasov–Maxwell (HVM) model is presented and recent results about the link
between kinetic effects and turbulence are reviewed. Using five-dimensional (2D in space …
between kinetic effects and turbulence are reviewed. Using five-dimensional (2D in space …
Nature of kinetic scale turbulence in the Earth's magnetosheath
CHK Chen, S Boldyrev - The Astrophysical Journal, 2017 - iopscience.iop.org
We present a combined observational and theoretical analysis to investigate the nature of
plasma turbulence at kinetic scales in the Earth's magnetosheath. In the first decade of the …
plasma turbulence at kinetic scales in the Earth's magnetosheath. In the first decade of the …