Dynamics and Structure of Quiescent Solar Prominences

Author:   E.R. Priest
Publisher:   Springer
Edition:   Softcover reprint of the original 1st ed. 1989
Volume:   150
ISBN:  

9789027728340


Pages:   217
Publication Date:   31 December 1988
Format:   Paperback
Availability:   Out of stock   Availability explained
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Dynamics and Structure of Quiescent Solar Prominences


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Author:   E.R. Priest
Publisher:   Springer
Imprint:   Kluwer Academic Publishers
Edition:   Softcover reprint of the original 1st ed. 1989
Volume:   150
Dimensions:   Width: 15.50cm , Height: 1.20cm , Length: 23.50cm
Weight:   0.720kg
ISBN:  

9789027728340


ISBN 10:   9027728348
Pages:   217
Publication Date:   31 December 1988
Audience:   College/higher education ,  Professional and scholarly ,  Postgraduate, Research & Scholarly ,  Professional & Vocational
Format:   Paperback
Publisher's Status:   Active
Availability:   Out of stock   Availability explained
The supplier is temporarily out of stock of this item. It will be ordered for you on backorder and shipped when it becomes available.

Table of Contents

1 Introduction to Quiescent Solar Prominences (E R Priest).- 1.1 Basic Description.- 1.2 Basic Equations of MHD.- 1.3 Prominence Puzzles.- 2 Overall Properties and Steady Flows (B Schmieder).- 2.1 Basic Properties.- 2.2 Physical Characteristics: Density and Temperature.- 2.3 Velocity Field and Mass Flux.- 2.4 Instability.- 2.5 Conclusion.- 3 Prominence Environment (O Engvold).- 3.1 Introduction.- 3.2 Helmet Streamers.- 3.3 Coronal Cavities.- 3.4 Filament Channels.- 3.5 Prominence-Corona Transition Region.- 3.6 Prominences and Environment.- 3.7 Modelling of the Helmet Streamer/Prominence Complex.- 3.8 Conclusions.- 4 Observation of Prominence Magnetic Fields (J L Leroy).- 4.1 Historical Steps.- 4 2 Investigations Based on the Polarimetry of Spectral Lines.- 4.3 Indirect Magnetic Field Determinations.- 4.4 Magnetic Field at the Photospheric Level.- 4.5 Main Features of the Magnetic Field in Quiescent Prominences.- 4.6 Some Important Problems.- 5 The Formation of Solar Prominences (J M Malherbe).- 5.1 Introduction.- 5.2 Overview of Observations.- 5.3 Main MHD Instabilities Involved in Prominence Formation.- 5.4 Steady Reconnection in Current Sheets.- 5.5 Static Models.- 5.6 Dynamic Models: Injection from the Chromosphere into Closed Loops.- 5.7 Dynamic Models: Condensation in Coronal Current Sheets.- 5.8 Unsolved Problems.- 5.9 Conclusion.- 6 Structure and Equilibrium of Prominences (U Anzer).- 6.1 Introduction.- 6.2 Prominence Models.- 6.3 Concluding Remarks.- 7 Stability and Eruption of Prominences (A W Hood).- 7.1 Introduction.- 7.2 Description of MHD Instabilities.- 7.3 Methods of Solution.- 7.4 Effect of the Dense Photosphere.- 7.5 Coronal Arcades.- 7.6 Thermal Stability.- 7.7 Resistive Instabilities — Tearing Modes.- 7.8 Simple Model of Prominence Eruption and aCoronal Mass Ejection.- 7.9 Conclusions and Future Work.- References.

Reviews

This book is a wonderful contribution from the European solar physics community.' Space Sciences Review 61, 1992 It certainly belongs in libraries or in the personal collection of a specialist.' American Scientist, 78


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