Turbulent Proton Heating Rate in the Solar Wind from 5–45 R ⊙
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/abfcd1/pdf
Reference67 articles.
1. A Solar Coronal Hole and Fast Solar Wind Turbulence Model and First-orbit Parker Solar Probe (PSP) Observations
2. Radio synthesis imaging of anisotropic angular broadening in the solar wind
3. Observations of field-aligned density fluctuations in the inner solar wind
4. Measurement of the Electric Fluctuation Spectrum of Magnetohydrodynamic Turbulence
5. Enhanced Energy Transfer Rate in Solar Wind Turbulence Observed near the Sun from Parker Solar Probe
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1. Estimates of Proton and Electron Heating Rates Extended to the Near-Sun Environment;The Astrophysical Journal Letters;2023-09-26
2. Coronal Heating Rate in the Slow Solar Wind;The Astrophysical Journal Letters;2023-09-01
3. Preparing for solar and heliospheric science with the SKAO: An Indian perspective;Journal of Astrophysics and Astronomy;2023-04-28
4. Direct observation of solar wind proton heating from in situ plasma measurements;Astronomy & Astrophysics;2023-04-27
5. Observations of cross scale energy transfer in the inner heliosphere by Parker Solar Probe;Reviews of Modern Plasma Physics;2022-11-23
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