Magnetospheric Cusps: Structure and Dynamics

Name: Magnetospheric Cusps: Structure and Dynamics
Brand: Springer
SKU: 9789048168651
Price: 2286 CZK
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Autor: Theodore A. Fritz, Shing F. Fung

Jazyk:

Vazba: Brožovaná

Vydavatel: Springer

Dostupnost: Skladem u dodavatele

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2 286 Kč

This collection of papers will address the question "What is the Magnetospheric Cusp?" and what is i...

Informace o knize

Autor

Theodore A. Fritz, Shing F. Fung

Jazyk

Angličtina

Vazba

Kniha - Brožovaná

Vydáno

2010

Stránek

414

EAN

9789048168651

ISBN

9048168651

Enbook ID

01975106

Vydavatel

Springer

Hmotnost

668

Rozměry

160 x 240 x 23

Kompletní popis

This collection of papers will address the question "What is the Magnetospheric Cusp?" and what is its role in the coupling of the solar wind to the magnetosphere as well as its role in the processes of particle transport and energization within the magnetosphere. The cusps have traditionally been described as narrow funnel-shaped regions that provide a focus of the Chapman-Ferraro currents that flow on the magnetopause, a boundary between the cavity dominated by the geomagnetic field (i.e., the magnetosphere) and the external region of the interplanetary medium. Measurements from a number of recent satellite programs have shown that the cusp is not confined to a narrow region near local noon but appears to encompass a large portion of the dayside high-latitude magnetosphere. It appears that the cusp is a major source region for the production of energetic charged particles for the magnetosphere.§This book will be of great interest to scientists in Space Physics as well as to those working in research organizations in governments and industries, university departments of physics, astronomy, space physics, and geophysics. Part of this book has already been published in a journal.This collection of papers will address the question "What is the Magnetospheric Cusp?" and what is its role in the coupling of the solar wind to the magnetosphere as well as its role in the processes of particle transport and energization within the magnetosphere. The cusps have traditionally been described as narrow funnel-shaped regions that provide a focus of the Chapman-Ferraro currents that flow on the magnetopause, a boundary between the cavity dominated by the geomagnetic field (i.e., the magnetosphere) and the external region of the interplanetary medium. Measurements from a number of recent satellite programs have shown that the cusp is not confined to a narrow region near local noon but appears to encompass a large portion of the dayside high-latitude magnetosphere and it appears that the cusp is a major source region for the production of energetic charged particles for the magnetosphere.§Audience:§This book will be of interest to space science research organizations in governments and industries, the community of Space Physics scientists and university departments of physics, astronomy, space physics, and geophysics.

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