Turbulent Heating and Anisotropy in the Solar Wind - A Numerical Study (Hardcover, 1st ed. 2019)

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 Alfven 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 Alfven 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.

General

Imprint:	Springer Nature Switzerland AG
Country of origin:	Switzerland
Series:	Springer Theses
Release date:	October 2019
First published:	2019
Authors:	Victor Montagud-Camps
Dimensions:	235 x 155mm (L x W)
Format:	Hardcover
Pages:	123
Edition:	1st ed. 2019
ISBN-13:	978-3-03-030382-2
Categories:	Books > Science & Mathematics > Astronomy, space & time > Theoretical & mathematical astronomy Books > Science & Mathematics > Astronomy, space & time > Solar system > General Books > Professional & Technical > Other technologies > Space science > Astronautics Promotions
LSN:	3-03-030382-9
Barcode:	9783030303822

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