[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares ar… Mehr…
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists. 262 pp. Englisch, Books<
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[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares ar… Mehr…
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists. 262 pp. Englisch, Books<
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BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Germany [57449362] [Rating: 5 (von 5)] NEW BOOK. Versandkosten:Versandkostenfrei. (EUR 0.00) Details...
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[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares ar… Mehr…
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists. 262 pp. Englisch, Books<
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[EAN: 9780792312611], Neubuch, [SC: 0.0], [PU: Springer Netherlands], ASTROPHYSIK; PHYSIK / CORONA; ARE, Druck auf Anfrage Neuware - Printed after ordering - Solar flares are very complex… Mehr…
[EAN: 9780792312611], Neubuch, [SC: 0.0], [PU: Springer Netherlands], ASTROPHYSIK; PHYSIK / CORONA; ARE, Druck auf Anfrage Neuware - Printed after ordering - Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists., Books<
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands], ASTROPHYSIK PHYSIK CORONA ARE ASTRONOMIE SOLAR FLARE ASTROPHYSICS AND ASTROPARTICLES, Dieser Artikel ist ein Print on Demand Art… Mehr…
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands], ASTROPHYSIK PHYSIK CORONA ARE ASTRONOMIE SOLAR FLARE ASTROPHYSICS AND ASTROPARTICLES, Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of t., Books<
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares ar… Mehr…
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists. 262 pp. Englisch, Books<
NEW BOOK. Versandkosten:Versandkostenfrei. (EUR 0.00) BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Germany [57449362] [Rating: 4 (von 5)]
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares ar… Mehr…
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists. 262 pp. Englisch, Books<
NEW BOOK. Versandkosten:Versandkostenfrei. (EUR 0.00) BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Germany [57449362] [Rating: 5 (von 5)]
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares ar… Mehr…
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands Dez 1991], ASTROPHYSIK; PHYSIK / CORONA; ARE, This item is printed on demand - it takes 3-4 days longer - Neuware -Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists. 262 pp. Englisch, Books<
NEW BOOK. Versandkosten:Versandkostenfrei. (EUR 0.00) BuchWeltWeit Inh. Ludwig Meier e.K., Bergisch Gladbach, Germany [57449362] [Rating: 5 (von 5)]
[EAN: 9780792312611], Neubuch, [SC: 0.0], [PU: Springer Netherlands], ASTROPHYSIK; PHYSIK / CORONA; ARE, Druck auf Anfrage Neuware - Printed after ordering - Solar flares are very complex… Mehr…
[EAN: 9780792312611], Neubuch, [SC: 0.0], [PU: Springer Netherlands], ASTROPHYSIK; PHYSIK / CORONA; ARE, Druck auf Anfrage Neuware - Printed after ordering - Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists., Books<
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands], ASTROPHYSIK PHYSIK CORONA ARE ASTRONOMIE SOLAR FLARE ASTROPHYSICS AND ASTROPARTICLES, Dieser Artikel ist ein Print on Demand Art… Mehr…
[EAN: 9780792312611], Neubuch, [PU: Springer Netherlands], ASTROPHYSIK PHYSIK CORONA ARE ASTRONOMIE SOLAR FLARE ASTROPHYSICS AND ASTROPARTICLES, Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of t., Books<
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Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists.
Detailangaben zum Buch - Physical Processes in Solar Flares by B.V. Somov Hardcover | Indigo Chapters
EAN (ISBN-13): 9780792312611 ISBN (ISBN-10): 0792312619 Gebundene Ausgabe Erscheinungsjahr: 1991 Herausgeber: B.V. Somov 262 Seiten Gewicht: 0,561 kg Sprache: eng/Englisch
Buch in der Datenbank seit 2008-02-21T10:37:19+01:00 (Berlin) Detailseite zuletzt geändert am 2024-03-25T19:55:59+01:00 (Berlin) ISBN/EAN: 0792312619
ISBN - alternative Schreibweisen: 0-7923-1261-9, 978-0-7923-1261-1 Alternative Schreibweisen und verwandte Suchbegriffe: Autor des Buches: somov boris Titel des Buches: flares, physica 1990, sola 1969, edition solar, physical science, astrophysics and space science library
Daten vom Verlag:
Autor/in: B.V. Somov Titel: Astrophysics and Space Science Library; Physical Processes in Solar Flares Verlag: Springer; Springer Netherland 249 Seiten Erscheinungsjahr: 1991-12-31 Dordrecht; NL Sprache: Englisch 160,49 € (DE) 164,99 € (AT) 177,00 CHF (CH) Available VIII, 249 p.
BB; Hardcover, Softcover / Physik, Astronomie/Astronomie; Astrophysik; Verstehen; Corona; Solar flare; solar; Astrophysics; BC
1 / The Present State of the Solar Problem.- 1.1.Observed phenomena and the energetics of solar flares.- 1.2.Physical concepts of the nature of flares.- 1.3.Flare-induced physical processes in the solar atmosphere.- 1.4.The solar flare problem.- 2 / Chromospheric Heating: The Mechanism Producing High-Temperature Plasma in Solar Flares.- 2.1.Impulsive heating by accelerated electrons.- 2.2.Impulsive heating by intense heat flows.- 2.3.Chromospheric heating by X-ray emission.- 3 / Magnetic Reconnection and Energy Release in Solar Flares.- 3.1.Reconnection as a heating mechanism for X-ray coronal loops.- 3.2.The natural high-temperature turbulent current sheet.- 3.3.The high-temperature turbulent current sheet with a small transverse magnetic field.- 3.4.The current sheet structure under the fast and slow reconnection regimes.- 3.5.Stabilization of tearing instability in current sheets on the Sun.- 3.6.The effect of the longitudinal magnetic field in the current sheets on the Sun.- Conclusion.- References.
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