Turbulent Heating and Anisotropy in the Solar Wind [E-Book] : A Numerical Study / by Victor Montagud-Camps.
This book presents two important new findings. First, it demonstrates from first principles that turbulent heating offers an explanation for the non-adiabatic decay of proton temperature in solar wind. Until now, this was only proved with reduced or phenomenological models. Second, the book demonstr...
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Full text |
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Personal Name(s): | Montagud-Camps, Victor, author |
Edition: |
1st edition 2019. |
Imprint: |
Cham :
Springer,
2019
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Physical Description: |
XVII, 123 pages 45 illustrations, 13 illustrations in color (online resource) |
Note: |
englisch |
ISBN: |
9783030303839 |
DOI: |
10.1007/978-3-030-30383-9 |
Series Title: |
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Springer Theses, Recognizing Outstanding Ph.D. Research
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Subject (LOC): |
- Introduction
- Solar Wind
- Plasma description
- Turbulence
- Solar Wind turbulence
- Plan of this thesis
- The Maltese Cross revisited
- Parameters and initial conditions
- Defining spectral properties in EBM simulations
- Results
- Discussion
- Can the Maltese Cross heat?
- Paper ApJ 2018: "Turbulent Heating between 0.2 and 1 au: A Numerical Study"
- Heating fast winds
- Conclusions and future work
- Conclusions
- Future work: Anisotropy temperature description
- Appendix.