Energetic Phenomena on the Sun: Astrophysics and Space Science Library, cartea 153
Editat de M. R. Kundu, B. Woodgate, E.J. Schmahlen Limba Engleză Hardback – 30 apr 1989
Toate formatele și edițiile | Preț | Express |
---|---|---|
Paperback (1) | 1213.31 lei 6-8 săpt. | |
SPRINGER NETHERLANDS – 23 aug 2014 | 1213.31 lei 6-8 săpt. | |
Hardback (1) | 1220.14 lei 6-8 săpt. | |
SPRINGER NETHERLANDS – 30 apr 1989 | 1220.14 lei 6-8 săpt. |
Din seria Astrophysics and Space Science Library
- 24% Preț: 799.08 lei
- 15% Preț: 637.00 lei
- 18% Preț: 967.22 lei
- 18% Preț: 776.96 lei
- Preț: 359.85 lei
- Preț: 389.70 lei
- 20% Preț: 691.13 lei
- 18% Preț: 994.20 lei
- Preț: 395.82 lei
- 15% Preț: 653.73 lei
- Preț: 391.48 lei
- 18% Preț: 938.66 lei
- Preț: 404.16 lei
- 18% Preț: 1204.61 lei
- 18% Preț: 1812.11 lei
- Preț: 386.56 lei
- Preț: 393.57 lei
- 18% Preț: 937.74 lei
- 18% Preț: 944.40 lei
- Preț: 391.69 lei
- Preț: 384.31 lei
- Preț: 406.83 lei
- Preț: 409.67 lei
- 18% Preț: 931.68 lei
- Preț: 397.73 lei
- 18% Preț: 940.37 lei
- Preț: 396.98 lei
- 18% Preț: 1208.64 lei
- 18% Preț: 1204.31 lei
- Preț: 397.53 lei
- 15% Preț: 643.73 lei
- 18% Preț: 1227.11 lei
- 18% Preț: 939.14 lei
- 18% Preț: 1815.05 lei
- 18% Preț: 1212.25 lei
- 18% Preț: 1213.92 lei
- Preț: 404.74 lei
Preț: 1220.14 lei
Preț vechi: 1487.98 lei
-18% Nou
Puncte Express: 1830
Preț estimativ în valută:
233.63€ • 241.00$ • 193.63£
233.63€ • 241.00$ • 193.63£
Carte tipărită la comandă
Livrare economică 20 februarie-06 martie
Preluare comenzi: 021 569.72.76
Specificații
ISBN-13: 9780792301721
ISBN-10: 0792301722
Pagini: 632
Ilustrații: XXVIII, 632 p.
Dimensiuni: 156 x 234 x 40 mm
Greutate: 1.12 kg
Ediția:1989
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria Astrophysics and Space Science Library
Locul publicării:Dordrecht, Netherlands
ISBN-10: 0792301722
Pagini: 632
Ilustrații: XXVIII, 632 p.
Dimensiuni: 156 x 234 x 40 mm
Greutate: 1.12 kg
Ediția:1989
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria Astrophysics and Space Science Library
Locul publicării:Dordrecht, Netherlands
Public țintă
ResearchCuprins
1: Preflare Activity.- 1.1 Introduction.- 1.2 Magnetohydrodynamic Instability..- 1.3 Preflare Magnetic and Velocity Fields.- 1.4 Coronal Manifestations of Preflare Activity.- 1.5 References.- 2: Particle Acceleration.- 2.1 Introduction.- 2.2 Phenomena Associated with Mildly-Relativistic Electrons.- 2.3 Phenomena Associated with Ions and Relativistic Electrons in Solar Flares.- 2.4 Theoretical Studies Of Particle Acceleration.- 2.5 Achievements — Outstanding Questions.- 2.6 Acknowledgements.- 2.7 References.- 3: Impulsive Phase Transport.- 3.1 Introduction.- 3.2 Impulsive Phase Observations and their Interpretation.- 3.3 Theoretical Studies of Transport Processes.- 3.4 Summary.- 3.5 References.- 4: Chromospheric Explosions.- 4.1 Introduction.- 4.2 Crystal Spectrometer Experiments.- 4.3 Debate of Issue 1.- 4.4 Debate of Issue 2.- 4.5 Debate of Issue 3.- 4.6 References.- 5: Flare Energetics.- 5.1 Introduction.- 5.2 Energetics of the Impulsive Phase.- 5.3 The Energetics of the Gradual Phase.- 5.4 Relationships among the Phases.- 5.5 Characterization of Total Flare Energy.- 5.6 Conclusions.- 5A. Flares Chosen for the Energetics Study.- 5B. A Review of Impulsive Phase Phenomena.- 5.7 Acknowledgements.- 5.8. References.- 6: Coronal Mass Ejections and Coronal Structures.- 6.1 Intrdocution.- 6.2 Observations.- 6.3 The Initiation of Coronal Mass Ejections.- 6.4 Modelling of Coronal Mass Ejections and Post-Flare Arches.- 6.5 Interplanetary Effects of Coronal Mass Ejections.- 6.6 The Slowly Varying Corona Near Solar Activity Maximum.- 6.6 Summary.- 6.7 Acknowledgements.- 6.8 References.- 7: Intercomparison of Numerical Models of Flaring Coronal Loops.- 7.1 Introduction.- 7.2 The Original Benchmark Problem.- 7.3 Initial Solution Comparisons.- 7.4 Final Benchmark Problem andSolution Comparison.- 7.5 Conclusions.- 7.6 References.- SMM Participants.