THREE-DIMENSIONAL STRUCTURE OF SOLAR WIND TURBULENCE-Reference-Cited by-同舟云学术

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THREE-DIMENSIONAL STRUCTURE OF SOLAR WIND TURBULENCE

Published:2012-10-08 Issue:2 Volume:758 Page:120
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Chen C. H. K.,Mallet A.,Schekochihin A. A.,Horbury T. S.,Wicks R. T.,Bale S. D.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/758/i=2/a=120/pdf

Reference71 articles.

1. Spectra and anisotropy of magnetic fluctuations in the Earth's magnetosheath: Cluster observations

2. Existence of Electromagnetic-Hydrodynamic Waves

3. Measurement of the Electric Fluctuation Spectrum of Magnetohydrodynamic Turbulence

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1. Anisotropy of Magnetohydrodynamic and Kinetic Scale Fluctuations through Correlation Tensor in Solar Wind at 0.8 au;Fractal and Fractional;2024-06-14

2. Anisotropy of Density Fluctuations in the Solar Wind at 1 au;The Astrophysical Journal;2024-05-29

3. Simultaneously Interactions of Ultra‐Low‐Frequency Waves and Whistler Waves, and Whistler Waves and Quasi‐Electrostatic Whistler Harmonics in the Earth's Magnetosheath;Journal of Geophysical Research: Space Physics;2024-05

4. HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence;Space Science Reviews;2023-11-03

5. Properties Underlying the Variation of the Magnetic Field Spectral Index in the Inner Solar Wind;The Astrophysical Journal;2023-11-01

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