Sun : A Laboratory for Astrophysics

NATO Advanced Study Institute on the Sun: a Laboratory for Astrophysics (1991 : Crieff, Scotland); Brown, John C. (EDT); Schmelz, Joan T.; North Atlantic Treaty Organization. Scientific Affairs Division (COR)

ISBN 10: 0792318110 ISBN 13: 9780792318118
Editore: Springer, 1992
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As in the days following Skylab, solar physics came to the end of an era when the So­ lar Maximum Mission re-entered the earth's atmosphere in December 1989. The 1980s had been a pioneering decade not only in space- and ground-based studies of the solar atmosphere (Solar Maximum Mission, Hinotori, VLA, Big Bear, Nanc;ay, etc.) but also in solar-terrestrial relations (ISEE, AMPTE), and solar interior neutrino and helioseismol­ ogy studies. The pace of development in related areas of theory (nuclear, atomic, MHD, beam-plasma) has been equally impressive. All of these raised tantalizing further questions about the structure and dynamics of the Sun as the prototypical and best observed star. This Advanced Study Institute was timed at a pivotal point between that decade and the realisation of Yohkoh, Ulysses, SOHO, GRANAT, Coronas, and new ground-based optical facilities such as LEST and GONG, so as to teach and inspire the up and coming young solar researchers of the 1990s. The topics, lecturers, and students were all chosen with this goal in mind, and the result seems to have been highly successful by all reports.

Contenuti: Preface. 1. Opening Address; J.C. Brown. Part I: Solar Interior. 2. The Structure and Evolution of the Sun; J. Christensen-Dalsgaard. 3. Seismic Investigation of the Solar Interior; J. Christensen-Dalsgaard. 4. Convection; M. Schüssler. 5. Mean Field Dynamo Theory; P. Hoyng. 6. The MHD Description of Cosmic Plasmas; K. Tsinganos. 7. Symmetric and Nonsymmetric MHD Equilibria; K. Tsinganos. Part II: Solar and Stellar Atmospheres. 8. The Photosphere; H. Zirin. 9. Small-Scale Photospheric Magnetic Fields; M. Schüssler. 10. Sunspots: A Laboratory for Solar Physics; J.B. Gurman. 11. Chromospheric Structure; J.B. Gurman. 12. Spectroscopic Diagnostics; A.H. Gabriel. 13. The Solar Corona; A.H. Gabriel. 14. Solar Radio Observations; G.J. Hurford. 15. Stellar Chromospheres, Coronae, and Winds; R. Pallavicini. 16. Exact 2-D MHD Solutions for Astrophysical Outflows; K. Tsinganos, E. Trussoni, C. Sauty. Part III: Solar Instrumentation. 17. Solar Optical Instrumentation; H. Zirin. 18. Solar Ultraviolet Instrumentation; J.B. Gurman. 19. Solar Radio Instrumentation; G.J. Hurford. 20. Soft X-Ray Instrumentation; A.H. Gabriel. 21. X-Ray Instrumentation; G.J. Hurford. Part IV: Solar and Stellar Activity. 22. Solar Activity; H. Zirin. 23. Overview of Solar Flares; A.G. Emslie. 24.High-Energy Flare Emissions; A.G. Emslie. 25. Energy Release and Transport in Flare Plasmas; A.G. Emslie. 26. Stellar Flares: Observations and Modelling; R. Pallavicini. 27. Physics of Flares in Stars and Accretion Disks; J. Kuijpers. Index.

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Titolo: Sun : A Laboratory for Astrophysics
Casa editrice: Springer
Data di pubblicazione: 1992
Legatura: Rilegato
Condizione: New

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Buch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -As in the days following Skylab, solar physics came to the end of an era when the So lar Maximum Mission re-entered the earth's atmosphere in December 1989. The 1980s had been a pioneering decade not only in space- and ground-based studies of the solar atmosphere (Solar Maximum Mission, Hinotori, VLA, Big Bear, Nanc;ay, etc.) but also in solar-terrestrial relations (ISEE, AMPTE), and solar interior neutrino and helioseismol ogy studies. The pace of development in related areas of theory (nuclear, atomic, MHD, beam-plasma) has been equally impressive. All of these raised tantalizing further questions about the structure and dynamics of the Sun as the prototypical and best observed star. This Advanced Study Institute was timed at a pivotal point between that decade and the realisation of Yohkoh, Ulysses, SOHO, GRANAT, Coronas, and new ground-based optical facilities such as LEST and GONG, so as to teach and inspire the up and coming young solar researchers of the 1990s. The topics, lecturers, and students were all chosen with this goal in mind, and the result seems to have been highly successful by all reports. 636 pp. Englisch. Codice articolo 9780792318118

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Buch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -As in the days following Skylab, solar physics came to the end of an era when the So lar Maximum Mission re-entered the earth's atmosphere in December 1989. The 1980s had been a pioneering decade not only in space- and ground-based studies of the solar atmosphere (Solar Maximum Mission, Hinotori, VLA, Big Bear, Nanc;ay, etc.) but also in solar-terrestrial relations (ISEE, AMPTE), and solar interior neutrino and helioseismol ogy studies. The pace of development in related areas of theory (nuclear, atomic, MHD, beam-plasma) has been equally impressive. All of these raised tantalizing further questions about the structure and dynamics of the Sun as the prototypical and best observed star. This Advanced Study Institute was timed at a pivotal point between that decade and the realisation of Yohkoh, Ulysses, SOHO, GRANAT, Coronas, and new ground-based optical facilities such as LEST and GONG, so as to teach and inspire the up and coming young solar researchers of the 1990s. The topics, lecturers, and students were all chosen with this goal in mind, and the result seems to have been highly successful by all reports.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 636 pp. Englisch. Codice articolo 9780792318118

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Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - As in the days following Skylab, solar physics came to the end of an era when the So lar Maximum Mission re-entered the earth's atmosphere in December 1989. The 1980s had been a pioneering decade not only in space- and ground-based studies of the solar atmosphere (Solar Maximum Mission, Hinotori, VLA, Big Bear, Nanc;ay, etc.) but also in solar-terrestrial relations (ISEE, AMPTE), and solar interior neutrino and helioseismol ogy studies. The pace of development in related areas of theory (nuclear, atomic, MHD, beam-plasma) has been equally impressive. All of these raised tantalizing further questions about the structure and dynamics of the Sun as the prototypical and best observed star. This Advanced Study Institute was timed at a pivotal point between that decade and the realisation of Yohkoh, Ulysses, SOHO, GRANAT, Coronas, and new ground-based optical facilities such as LEST and GONG, so as to teach and inspire the up and coming young solar researchers of the 1990s. The topics, lecturers, and students were all chosen with this goal in mind, and the result seems to have been highly successful by all reports. Codice articolo 9780792318118

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Condizione: New. Proceedings of the NATO Advanced Study Institute, Crieff, Scotland, June 16-29, 1991 Editor(s): Schmelz, Joan T.; Brown, Richard J. C. Series: NATO Science Series C. Num Pages: 617 pages, biography. BIC Classification: PGS; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 234 x 156 x 34. Weight in Grams: 1061. . 1992. Hardback. . . . . Codice articolo V9780792318118

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Condizione: New. Proceedings of the NATO Advanced Study Institute, Crieff, Scotland, June 16-29, 1991 Editor(s): Schmelz, Joan T.; Brown, Richard J. C. Series: NATO Science Series C. Num Pages: 617 pages, biography. BIC Classification: PGS; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 234 x 156 x 34. Weight in Grams: 1061. . 1992. Hardback. . . . . Books ship from the US and Ireland. Codice articolo V9780792318118

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