The Role of Alfvén Wave Dynamics on the Large-scale Properties of the Solar Wind: Comparing an MHD Simulation with Parker Solar Probe E1 Data
Author:
Funder
NASA
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4365/ab4fef/pdf
Reference58 articles.
1. Magnetic fields and the structure of the solar corona
2. Radiation loss rates in Lyman-alpha for solar conditions
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