Convection and Substorms

Name: Convection and Substorms
Brand: Oxford University Press Inc
SKU: 9780195085297
Price: 132.31 EUR
Availability: InStock

Paradigms of Magnetospheric Phenomenology

Автор: Charles F. Kennel

Език:

Корици: С твърди корици

Издател: Oxford University Press Inc

Наличност: Външен склад

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132.31 € 258.77 лв

The magnetosphere is the region in which the solar wind interacts with the Earth's magnetic field, t...

Информация за книгата

Автор

Charles F. Kennel

Език

Английски език

Корици

Книга - С твърди корици

Издадена

1996

страници

428

EAN

9780195085297

ISBN

0195085299

Enbook ID

04513224

Издател

Oxford University Press Inc

Теглоt

781

Размери

163 x 243 x 34

Пълно описание

The magnetosphere is the region in which the solar wind interacts with the Earth's magnetic field, the zone which screens the Earth from most of the harmful cosmic rays which daily bombard it. The Aurora Borealis, or Norhun lights, other such phenourena result from the interaction of particles in the solar wind and the magnetosphere. Planetary physicists, geophysicists, plasma astrophysicists, and scientists involved with astronautics all have a primary interest in the configuration and dynamics of the magnetosphere, and much research is devoted to convection (the circulation of solarwind plasma in the magnetiosphere) and substorms, which are linked to the aurorae and thought to stimulate convection. In this book, one of the leading scientists in the field presents a synthesis of current knowledge on convection and substorms and proposes that the steady reconnection model be replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.

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Convection and Substorms

Paradigms of Magnetospheric Phenomenology

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