Turbulent Heating and Anisotropy in the Solar Wind A Numerical Study /
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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| Format: | Electronic eBook |
| Language: | English |
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Cham :
Springer International Publishing : Imprint: Springer,
2019.
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| Edition: | 1st ed. 2019. |
| Series: | Springer Theses, Recognizing Outstanding Ph.D. Research,
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| Online Access: | Full Text via HEAL-Link |
Table of Contents:
- 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.