RECONNECTION OUTFLOW GENERATED TURBULENCE IN THE SOLAR WIND
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.1088/2041-8205/797/1/L10/pdf
Reference31 articles.
1. Universality of Solar-Wind Turbulent Spectrum from MHD to Electron Scales
2. Magnetic Fluctuation Power Near Proton Temperature Anisotropy Instability Thresholds in the Solar Wind
3. ON SPECTRAL BREAKS IN THE POWER SPECTRA OF MAGNETIC FLUCTUATIONS IN FAST SOLAR WIND BETWEEN 0.3 AND 0.9 AU
4. RADIAL DEPENDENCE OF THE FREQUENCY BREAK BETWEEN FLUID AND KINETIC SCALES IN THE SOLAR WIND FLUCTUATIONS
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1. Kinetic Scale Magnetic Reconnection with a Turbulent Forcing: Particle-in-cell Simulations;The Astrophysical Journal;2023-01-31
2. Solar Wind Turbulence Outlined Through Magnetic Islands and Nonlinear Waves;Frontiers in Astronomy and Space Sciences;2022-06-16
3. Turbulence-driven magnetic reconnection and the magnetic correlation length: Observations from Magnetospheric Multiscale in Earth's magnetosheath;Physics of Plasmas;2022-01
4. Magnetic Reconnection Within the Boundary Layer of a Magnetic Cloud in the Solar Wind;Journal of Geophysical Research: Space Physics;2021-09
5. Nonlinear evolution of dispersive Alfvén waves and the effect of magnetic islands in the solar wind plasmas;Physics of Plasmas;2020-07
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