Turbulent Heating and Anisotropy in the Solar Wind is popular PDF and ePub book, written by Victor Montagud-Camps in 2019-10-11, it is a fantastic choice for those who relish reading online the Science genre. Let's immerse ourselves in this engaging Science book by exploring the summary and details provided below. Remember, Turbulent Heating and Anisotropy in the Solar Wind can be Read Online from any device for your convenience.
Turbulent Heating and Anisotropy in the Solar Wind Book PDF Summary
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 demonstrates that the two types of anisotropy of turbulent fluctuations that are observed in solar wind at 1AU originate not only from two distinct classes of conditions near the Sun but also from the imbalance in Alfvén wave populations. These anisotropies do not affect the overall turbulent heating if we take into account the relation observed in solar wind between anisotropy and Alfvén wave imbalance. In terms of the methods used to obtain these achievements, the author shows the need to find a very delicate balance between turbulent decay and expansion losses, so as to directly solve the magnetohydrodynamic equations, including the wind expansion effects.
Detail Book of Turbulent Heating and Anisotropy in the Solar Wind PDF
- Author : Victor Montagud-Camps
- Release : 11 October 2019
- Publisher : Springer Nature
- ISBN : 9783030303839
- Genre : Science
- Total Page : 123 pages
- Language : English
- PDF File Size : 12,8 Mb
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