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 …
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
[HTML][HTML] The multi-scale nature of the solar wind
D Verscharen, KG Klein, BA Maruca - Living Reviews in Solar Physics, 2019 - Springer
The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …
associated with its characteristic spatial and temporal scales. The characteristic length …
Reconnection-driven energy cascade in magnetohydrodynamic turbulence
Magnetohydrodynamic turbulence regulates the transfer of energy from large to small scales
in many astrophysical systems, including the solar atmosphere. We perform three …
in many astrophysical systems, including the solar atmosphere. We perform three …
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 …
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 …
The properties of the solar corona and its connection to the solar wind
SR Cranmer, AR Winebarger - Annual Review of Astronomy …, 2019 - annualreviews.org
The corona is a layer of hot plasma that surrounds the Sun, traces out its complex magnetic
field, and ultimately expands into interplanetary space as the supersonic solar wind …
field, and ultimately expands into interplanetary space as the supersonic solar wind …
Properties of the turbulence associated with electron-only magnetic reconnection in Earth's magnetosheath
Turbulent plasmas generate intense current structures, which have long been suggested as
magnetic reconnection sites. Recent Magnetospheric Multiscale observations in Earth's …
magnetic reconnection sites. Recent Magnetospheric Multiscale observations in Earth's …
Turbulent magnetic reconnection generated by intense lasers
Y Ping, J Zhong, X Wang, B Han, W Sun, Y Zhang… - Nature Physics, 2023 - nature.com
Turbulent magnetic reconnection is believed to occur in astrophysical plasmas, and it has
been suggested to be a trigger of solar flares. It often occurs in long stretched and …
been suggested to be a trigger of solar flares. It often occurs in long stretched and …
Fully kinetic simulation of 3D kinetic Alfvén turbulence
We present results from a three-dimensional particle-in-cell simulation of plasma turbulence,
resembling the plasma conditions found at kinetic scales of the solar wind. The spectral …
resembling the plasma conditions found at kinetic scales of the solar wind. The spectral …
[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 …