Turbulence, Waves and Instabilities in the Solar Plasma Proceedings of the NATO Advanced Research Workshop on Turbulence, Waves, and Instabilities in the Solar Plasma Lillafured, Hungary 16–20 September 2002

Significant advances have been made recently in both the theoretical understanding and observation of small-scale turbulence in different layers of the Sun, and in the instabilities that give rise to them. The general development of solar physics, however, has led to such a degree of specialization...

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Bibliographic Details
Other Authors: Erdélyi, R. (Editor), Petrovay, K. (Editor), Roberts, B. (Editor), Aschwanden, Markus (Editor)
Format: eBook
Language:English
Published: Dordrecht Springer Netherlands 2003, 2003
Edition:1st ed. 2003
Series:NATO Science Series II: Mathematics, Physics and Chemistry, Mathematics, Physics and Chemistry
Subjects:
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
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245 0 0 |a Turbulence, Waves and Instabilities in the Solar Plasma  |h Elektronische Ressource  |b Proceedings of the NATO Advanced Research Workshop on Turbulence, Waves, and Instabilities in the Solar Plasma Lillafured, Hungary 16–20 September 2002  |c edited by R. Erdélyi, K. Petrovay, B. Roberts, Markus Aschwanden 
250 |a 1st ed. 2003 
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505 0 |a One / Instabilities and Motions in the Solar Interior and Tachocline -- A dynamo in the radiative interior -- Turbulence and its Sources Below the Convective Zone -- MHD simulations of small and large scale dynamos -- Two / Turbulence in the Convective Zone and Photosphere -- Helioseismic observations of plasma motions in the solar convection zone -- Turbulent Transport in Rotating and Magnetized Fluids -- Three / Parker Instability and Flux Tube Dynamics -- Three-dimensional Evolution of a Magnetic Flux Tube Emerging into the Solar Atmosphere -- Photospheric magnetic field at small scales -- Four / Waves and Oscillations in the Solar Atmosphere -- Waves in the chromosphere: observations -- Theory of MHD Waves in the Solar Corona -- Prominence Oscillations: Theory -- Review of Coronal Oscillations — An Observer’s View -- Nonlinear Waves in the Magnetically Structured Solar Atmosphere -- Five / Turbulence and Reconnection in the Solar Corona -- TRACE and Ground-based Observations of Small-scale Dynamics in Active Regions -- Observational Signatures of Magnetic Reconnection -- Self-organized Structures in the Solar Atmosphere: Theory and Observations -- Six / Solar Wind -- Wave Heating and Acceleration of the Fast Solar Wind -- Waves and turbulence in the solar wind 
653 |a Classical and Continuum Physics 
653 |a Nuclear physics 
653 |a Nuclear Physics 
653 |a Physics 
653 |a Astrophysics 
700 1 |a Petrovay, K.  |e [editor] 
700 1 |a Roberts, B.  |e [editor] 
700 1 |a Aschwanden, Markus  |e [editor] 
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520 |a Significant advances have been made recently in both the theoretical understanding and observation of small-scale turbulence in different layers of the Sun, and in the instabilities that give rise to them. The general development of solar physics, however, has led to such a degree of specialization as to hinder interaction between workers in the field. This book therefore presents studies of different layers and regions of the Sun, but from the same aspect, concentrating on the study of small-scale motions. The main emphasis is on the common theoretical roots of these phenomena, but the book also contains an extensive treatment of the observational aspects