Wave Composition, Propagation, and Polarization of Magnetohydrodynamic Turbulence within 0.3 au as Observed by Parker Solar Probe
Author:
Funder
NSFC
CNSA
STFC
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/abb23e/pdf
Reference51 articles.
1. Highly structured slow solar wind emerging from an equatorial coronal hole
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3. Observations of Energetic-particle Population Enhancements along Intermittent Structures near the Sun from the Parker Solar Probe
4. Collisionless Damping of Hydromagnetic Waves
5. Statistical properties of MHD fluctuations associated with high-speed streams from Helios-2 observations
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