Dynamics and Structure of Quiescent Solar Prominences: Astrophysics and Space Science Library, cartea 150
Editat de E. R. Priesten Limba Engleză Hardback – 31 dec 1988
Toate formatele și edițiile | Preț | Express |
---|---|---|
Paperback (1) | 637.28 lei 6-8 săpt. | |
SPRINGER NETHERLANDS – 31 dec 1988 | 637.28 lei 6-8 săpt. | |
Hardback (1) | 643.48 lei 6-8 săpt. | |
SPRINGER NETHERLANDS – 31 dec 1988 | 643.48 lei 6-8 săpt. |
Din seria Astrophysics and Space Science Library
- 24% Preț: 799.08 lei
- 15% Preț: 647.92 lei
- 18% Preț: 983.81 lei
- 18% Preț: 790.28 lei
- Preț: 359.85 lei
- Preț: 389.70 lei
- 20% Preț: 691.13 lei
- 18% Preț: 1011.27 lei
- Preț: 402.56 lei
- 15% Preț: 664.93 lei
- Preț: 398.15 lei
- 18% Preț: 954.77 lei
- Preț: 411.04 lei
- 18% Preț: 1225.31 lei
- 18% Preț: 1843.29 lei
- Preț: 393.13 lei
- Preț: 400.26 lei
- 18% Preț: 953.82 lei
- 18% Preț: 960.61 lei
- Preț: 398.35 lei
- Preț: 390.84 lei
- Preț: 413.76 lei
- Preț: 416.64 lei
- 18% Preț: 947.67 lei
- Preț: 404.51 lei
- 18% Preț: 956.50 lei
- Preț: 403.75 lei
- 18% Preț: 1229.40 lei
- 18% Preț: 1224.99 lei
- Preț: 404.29 lei
- 15% Preț: 654.77 lei
- 18% Preț: 1248.20 lei
- 18% Preț: 955.25 lei
- 18% Preț: 1846.28 lei
- 18% Preț: 1233.06 lei
- 18% Preț: 1234.77 lei
- Preț: 411.64 lei
Preț: 643.48 lei
Preț vechi: 757.04 lei
-15% Nou
Puncte Express: 965
Preț estimativ în valută:
123.14€ • 128.40$ • 102.34£
123.14€ • 128.40$ • 102.34£
Carte tipărită la comandă
Livrare economică 21 martie-04 aprilie
Preluare comenzi: 021 569.72.76
Specificații
ISBN-13: 9789027728333
ISBN-10: 902772833X
Pagini: 232
Ilustrații: X, 217 p.
Dimensiuni: 155 x 235 x 18 mm
Greutate: 0.5 kg
Ediția:1989
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria Astrophysics and Space Science Library
Locul publicării:Dordrecht, Netherlands
ISBN-10: 902772833X
Pagini: 232
Ilustrații: X, 217 p.
Dimensiuni: 155 x 235 x 18 mm
Greutate: 0.5 kg
Ediția:1989
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria Astrophysics and Space Science Library
Locul publicării:Dordrecht, Netherlands
Public țintă
ResearchCuprins
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.
Recenzii
`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
Space Sciences Review 61, 1992
`It certainly belongs in libraries or in the personal collection of a specialist.'
American Scientist, 78