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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Bibliographic Details
Main Author: Montagud-Camps, Victor (Author, http://id.loc.gov/vocabulary/relators/aut)
Corporate Author: SpringerLink (Online service)
Format: Electronic eBook
Language:English
Published: Cham : Springer International Publishing : Imprint: Springer, 2019.
Edition:1st ed. 2019.
Series:Springer Theses, Recognizing Outstanding Ph.D. Research,
Subjects:
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.