Name: Kelvin-Helmholtz Instability in Solar Atmospheric Jets (en Inglés)
Price: 453.15 PEN
Availability: InStock
Author: Zhelyazkov, Ivan ; Chandra, Ramesh
ISBN: 9789811223747

portada Kelvin-Helmholtz Instability in Solar Atmospheric Jets (en Inglés)

Formato

Libro Físico

Autor

Ivan Zhelyazkov

Ramesh Chandra

Editorial

World Scientific Publishing Company

Idioma

Inglés

N° páginas

256

Encuadernación

Tapa Dura

Dimensiones

22.9 x 15.2 x 1.6 cm

Peso

0.51 kg.

ISBN13

9789811223747

Categorías

Astronomía, espacio y tiempo
Electricidad, electromagnetismo y magnetismo
Astrofísica

Kelvin-Helmholtz Instability in Solar Atmospheric Jets (en Inglés)

Ivan Zhelyazkov (Autor) · Ramesh Chandra (Autor) · World Scientific Publishing Company · Tapa Dura

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S/ 453,15

S/ 906,29

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Origen: Estados Unidos (Costos de importación incluídos en el precio)

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Reseña del libro "Kelvin-Helmholtz Instability in Solar Atmospheric Jets (en Inglés)"

The book provides a comprehensive overview of the eruptive and wave phenomena in the solar atmosphere. One of the ongoing problems in solar physics is the heating of the solar corona. Currently there is a competition between two mechanisms in explaining the heating, i.e., dissipation of energy by waves and small scale frequent coronal magnetic reconnection. However, some studies indicate this may be a joint effect of these two possible mechanisms. Kelvin-Helmholtz Instability (KHI) of propagating magnetohydrodynamic modes in solar flowing structures plays an important role in the solar atmosphere. It can trigger the onset of wave turbulence leading to effective plasma heating and particle acceleration. KHI is a multifaceted phenomenon and the purpose of this book is to illuminate its (instability) manifestation in various solar jets like spicules, dark mottles, surges, macrospicules, Extreme Ultraviolet (EUV) and X-ray jets, as well as rotating, tornado-like, jets, solar wind, and coronal mass ejections.The modeling of KHI is performed in the framework of ideal magnetohydrodynamics. The book consists of 12 chapters and is intended primarily for advanced undergraduate and postgraduate students, as well as early career researchers.