Titlebook: Auroral Plasma Physics; Götz Paschmann,Stein Haaland,Rudolf Treumann Book 2003 Springer Science+Business Media Dordrecht 2003 HTS.Planet.R

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放气

Electrodynamics of Auroral Forms,ectrodynamics of these forms. By this we mean the local characteristics of the electric field, current, and conductivity patterns, and how these are interrelated. This relationship is governed by Ohm’s law, the requirement of current continuity, and use of field- aligned currents as the connecting a

大沟

Dynamic Coupling to the Magnetosphere,ions in auroral physics can be described within a quasi-static picture. However, even the most static arcs do dissipate energy and this energy dissipation must be supplied by an external energy source, which ultimately is the solar wind-magnetosphere interaction. The coupling, undoubtedly, is a dyna

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The Aurora as a Universal Phenomenon, to terrestrial auroral phenomena, but are of a very general nature. They take place in various different objects and places in the universe when magnetized plasmas of different constitution come into contact. Hot collisionless plasmas in convective motion connected via magnetic fields to cold colli

Omniscient

Nicola Luigi Bragazzi,Claudio NicoliniIn the previous Chapters we have presented many aspects of the morphology and microphysics of the aurora. The purpose of the present chapter is to describe theoretical models that try to put these into wider context. As there is yet no model that encompasses all aspects, the chapter will necessarily be rather heterogeneous.

Prologue

Theoretical Models,In the previous Chapters we have presented many aspects of the morphology and microphysics of the aurora. The purpose of the present chapter is to describe theoretical models that try to put these into wider context. As there is yet no model that encompasses all aspects, the chapter will necessarily be rather heterogeneous.

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Obesity and Genomics in the Netherlandseir emotional impression, the auroral phenomena have excited the curiosity of scientists since the days of Galileo. The rapid expansion of our capacity to observe the auroral processes, both remotely and in situ, has provided an enormous amount of data, which we are trying to organize and explain in

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