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Verlag: Springer Nature B.V., 2023
ISBN 10: 9402421971ISBN 13: 9789402421972
Anbieter: PBShop.store US, Wood Dale, IL, USA
Buch Print-on-Demand
PAP. Zustand: New. New Book. Shipped from UK. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.
Verlag: Springer, 2023
ISBN 10: 9402421971ISBN 13: 9789402421972
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
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Zustand: New. In English.
Verlag: Springer Nature B.V., 2023
ISBN 10: 9402421971ISBN 13: 9789402421972
Anbieter: PBShop.store UK, Fairford, GLOS, Vereinigtes Königreich
Buch Print-on-Demand
PAP. Zustand: New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.
Verlag: Springer, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: GreatBookPrices, Columbia, MD, USA
Buch
Zustand: New.
Verlag: Springer, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: booksXpress, Bayonne, NJ, USA
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Soft Cover. Zustand: new.
Verlag: Springer, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: GreatBookPrices, Columbia, MD, USA
Buch
Zustand: As New. Unread book in perfect condition.
Verlag: Springer Netherlands Jan 2023, 2023
ISBN 10: 9402421955ISBN 13: 9789402421958
Anbieter: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Deutschland
Buch Print-on-Demand
Buch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The book presents a broad and in-depth overview of recent achievements and the current state of research in magnetohydrodynamic (MHD) oscillatory and wave phenomena in the coronae of the Sun and stars. Major progress in coronal wave studies has been achieved thanks to the combination of high-precision multi-wavelength observations with spaceborne and ground-based facilities, elaborated theory of the interaction of MHD waves with plasma non-uniformities, state-of-the-art numerical simulations, and novel data analysis techniques. It has allowed the research community to reach a new look at the role played by MHD wave processes in the enigmatic phenomena of coronal plasma heating and wind acceleration as well as powerful energy releases such as flares and coronal mass ejections. In addition, the waves are intensively used as natural probes in the remote diagnostics of the coronal plasma parameters and physical processes operating in solar and stellar coronae via the method of MHD seismology. Individual chapters cover recent cutting-edge results obtained on the analysis and theoretical modelling of several most intensively studied coronal MHD wave phenomena, namely, kink and sausage oscillations of coronal loops and other field-aligned plasma structures, plus running and standing slow magnetoacoustic waves. A dedicated chapter assesses the reliability of proposed theoretical mechanisms for heating of the coronal plasma by MHD waves. Another chapter summarizes the current state of our understanding of the physical mechanisms and observational properties of quasi-periodic pulsations in solar flares, considers their analogy with similar processes detected in stellar flares, and thus establishes solid ground for the further exploitation of the solar-stellar analogy. An important discussion of novel data analysis techniques designed recently for MHD seismology applications is presented in a devoted chapter. The direction of future advances in the designated research areas are discussed.The book is a spin-off from the Topical Collection 'Oscillatory Processes in Solar and Stellar Coronae' of the journal Space Science Reviews. 396 pp. Englisch.
Verlag: Springer Netherlands Jan 2024, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Deutschland
Buch Print-on-Demand
Taschenbuch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The book presents a broad and in-depth overview of recent achievements and the current state of research in magnetohydrodynamic (MHD) oscillatory and wave phenomena in the coronae of the Sun and stars. Major progress in coronal wave studies has been achieved thanks to the combination of high-precision multi-wavelength observations with spaceborne and ground-based facilities, elaborated theory of the interaction of MHD waves with plasma non-uniformities, state-of-the-art numerical simulations, and novel data analysis techniques. It has allowed the research community to reach a new look at the role played by MHD wave processes in the enigmatic phenomena of coronal plasma heating and wind acceleration as well as powerful energy releases such as flares and coronal mass ejections. In addition, the waves are intensively used as natural probes in the remote diagnostics of the coronal plasma parameters and physical processes operating in solar and stellar coronae via the method of MHD seismology. Individual chapters cover recent cutting-edge results obtained on the analysis and theoretical modelling of several most intensively studied coronal MHD wave phenomena, namely, kink and sausage oscillations of coronal loops and other field-aligned plasma structures, plus running and standing slow magnetoacoustic waves. A dedicated chapter assesses the reliability of proposed theoretical mechanisms for heating of the coronal plasma by MHD waves. Another chapter summarizes the current state of our understanding of the physical mechanisms and observational properties of quasi-periodic pulsations in solar flares, considers their analogy with similar processes detected in stellar flares, and thus establishes solid ground for the further exploitation of the solar-stellar analogy. An important discussion of novel data analysis techniques designed recently for MHD seismology applications is presented in a devoted chapter. The direction of future advances in the designated research areas are discussed.The book is a spin-off from the Topical Collection 'Oscillatory Processes in Solar and Stellar Coronae' of the journal Space Science Reviews. 396 pp. Englisch.
Verlag: Springer, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: GreatBookPricesUK, Castle Donington, DERBY, Vereinigtes Königreich
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Zustand: New.
Verlag: Springer Netherlands 2024-01-11, Berlin, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: Blackwell's, London, Vereinigtes Königreich
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paperback. Zustand: New. Language: ENG.
Verlag: Springer, Dordrecht, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: Grand Eagle Retail, Wilmington, DE, USA
Buch Erstausgabe
Paperback. Zustand: new. Paperback. The book presents a broad and in-depth overview of recent achievements and the current state of research in magnetohydrodynamic (MHD) oscillatory and wave phenomena in the coronae of the Sun and stars. Major progress in coronal wave studies has been achieved thanks to the combination of high-precision multi-wavelength observations with spaceborne and ground-based facilities, elaborated theory of the interaction of MHD waves with plasma non-uniformities, state-of-the-art numerical simulations, and novel data analysis techniques. It has allowed the research community to reach a new look at the role played by MHD wave processes in the enigmatic phenomena of coronal plasma heating and wind acceleration as well as powerful energy releases such as flares and coronal mass ejections. In addition, the waves are intensively used as natural probes in the remote diagnostics of the coronal plasma parameters and physical processes operating in solar and stellar coronae via the method of MHD seismology. Individual chapters cover recent cutting-edge results obtained on the analysis and theoretical modelling of several most intensively studied coronal MHD wave phenomena, namely, kink and sausage oscillations of coronal loops and other field-aligned plasma structures, plus running and standing slow magnetoacoustic waves. A dedicated chapter assesses the reliability of proposed theoretical mechanisms for heating of the coronal plasma by MHD waves. Another chapter summarizes the current state of our understanding of the physical mechanisms and observational properties of quasi-periodic pulsations in solar flares, considers their analogy with similar processes detected in stellar flares, and thus establishes solid ground for the further exploitation of the solar-stellar analogy. An important discussion of novel data analysis techniques designed recently for MHD seismology applications is presented in a devoted chapter. The direction of future advances in the designated research areas are discussed.The book is a spin-off from the Topical Collection "Oscillatory Processes in Solar and Stellar Coronae" of the journal Space Science Reviews. Individual chapters cover recent cutting-edge results obtained on the analysis and theoretical modelling of several most intensively studied coronal MHD wave phenomena, namely, kink and sausage oscillations of coronal loops and other field-aligned plasma structures, plus running and standing slow magnetoacoustic waves. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.
Verlag: Springer, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: GreatBookPricesUK, Castle Donington, DERBY, Vereinigtes Königreich
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Zustand: As New. Unread book in perfect condition.
Verlag: Springer Netherlands, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: moluna, Greven, Deutschland
Buch Print-on-Demand
Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Gives a comprehensive overview of oscillatory processes in solar and stellar coronaeDiscusses observations made by primary instruments used to research solar and stellar phenomenaContains review, analysis, and modelling of cutting-edge rese.
Verlag: Springer Netherlands|Springer, 2023
ISBN 10: 9402421955ISBN 13: 9789402421958
Anbieter: moluna, Greven, Deutschland
Buch Print-on-Demand
Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. The book presents a broad and in-depth overview of recent achievements and the current state of research in magnetohydrodynamic (MHD) oscillatory and wave phenomena in the coronae of the Sun and stars. Major progress in coronal wave studies has been achieve.
Verlag: Springer, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: California Books, Miami, FL, USA
Buch
Zustand: New.
Verlag: Springer Netherlands, 2023
ISBN 10: 9402421955ISBN 13: 9789402421958
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The book presents a broad and in-depth overview of recent achievements and the current state of research in magnetohydrodynamic (MHD) oscillatory and wave phenomena in the coronae of the Sun and stars. Major progress in coronal wave studies has been achieved thanks to the combination of high-precision multi-wavelength observations with spaceborne and ground-based facilities, elaborated theory of the interaction of MHD waves with plasma non-uniformities, state-of-the-art numerical simulations, and novel data analysis techniques. It has allowed the research community to reach a new look at the role played by MHD wave processes in the enigmatic phenomena of coronal plasma heating and wind acceleration as well as powerful energy releases such as flares and coronal mass ejections. In addition, the waves are intensively used as natural probes in the remote diagnostics of the coronal plasma parameters and physical processes operating in solar and stellar coronae via the method of MHD seismology. Individual chapters cover recent cutting-edge results obtained on the analysis and theoretical modelling of several most intensively studied coronal MHD wave phenomena, namely, kink and sausage oscillations of coronal loops and other field-aligned plasma structures, plus running and standing slow magnetoacoustic waves. A dedicated chapter assesses the reliability of proposed theoretical mechanisms for heating of the coronal plasma by MHD waves. Another chapter summarizes the current state of our understanding of the physical mechanisms and observational properties of quasi-periodic pulsations in solar flares, considers their analogy with similar processes detected in stellar flares, and thus establishes solid ground for the further exploitation of the solar-stellar analogy. An important discussion of novel data analysis techniques designed recently for MHD seismology applications is presented in a devoted chapter. The direction of future advances in the designated research areas are discussed.The book is a spin-off from the Topical Collection 'Oscillatory Processes in Solar and Stellar Coronae' of the journal Space Science Reviews.
Verlag: Springer Netherlands, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch
Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The book presents a broad and in-depth overview of recent achievements and the current state of research in magnetohydrodynamic (MHD) oscillatory and wave phenomena in the coronae of the Sun and stars. Major progress in coronal wave studies has been achieved thanks to the combination of high-precision multi-wavelength observations with spaceborne and ground-based facilities, elaborated theory of the interaction of MHD waves with plasma non-uniformities, state-of-the-art numerical simulations, and novel data analysis techniques. It has allowed the research community to reach a new look at the role played by MHD wave processes in the enigmatic phenomena of coronal plasma heating and wind acceleration as well as powerful energy releases such as flares and coronal mass ejections. In addition, the waves are intensively used as natural probes in the remote diagnostics of the coronal plasma parameters and physical processes operating in solar and stellar coronae via the method of MHD seismology. Individual chapters cover recent cutting-edge results obtained on the analysis and theoretical modelling of several most intensively studied coronal MHD wave phenomena, namely, kink and sausage oscillations of coronal loops and other field-aligned plasma structures, plus running and standing slow magnetoacoustic waves. A dedicated chapter assesses the reliability of proposed theoretical mechanisms for heating of the coronal plasma by MHD waves. Another chapter summarizes the current state of our understanding of the physical mechanisms and observational properties of quasi-periodic pulsations in solar flares, considers their analogy with similar processes detected in stellar flares, and thus establishes solid ground for the further exploitation of the solar-stellar analogy. An important discussion of novel data analysis techniques designed recently for MHD seismology applications is presented in a devoted chapter. The direction of future advances in the designated research areas are discussed.The book is a spin-off from the Topical Collection 'Oscillatory Processes in Solar and Stellar Coronae' of the journal Space Science Reviews.
Verlag: Springer Nature, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: Revaluation Books, Exeter, Vereinigtes Königreich
Buch
Paperback. Zustand: Brand New. 393 pages. 9.25x6.10x1.38 inches. In Stock.
Verlag: Springer Nature, 2023
ISBN 10: 9402421955ISBN 13: 9789402421958
Anbieter: Revaluation Books, Exeter, Vereinigtes Königreich
Buch
Hardcover. Zustand: Brand New. 393 pages. 9.25x6.10x0.91 inches. In Stock.
Verlag: American Geophysical Union, 2016
ISBN 10: 1119054958ISBN 13: 9781119054955
Anbieter: GreatBookPricesUK, Castle Donington, DERBY, Vereinigtes Königreich
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Zustand: New.
Verlag: Amer Geophysical Union, 2016
ISBN 10: 1119054958ISBN 13: 9781119054955
Anbieter: GreatBookPrices, Columbia, MD, USA
Buch
Zustand: As New. Unread book in perfect condition.
Verlag: Springer, Dordrecht, 2024
ISBN 10: 940242198XISBN 13: 9789402421989
Anbieter: AussieBookSeller, Truganina, VIC, Australien
Buch Erstausgabe
Paperback. Zustand: new. Paperback. The book presents a broad and in-depth overview of recent achievements and the current state of research in magnetohydrodynamic (MHD) oscillatory and wave phenomena in the coronae of the Sun and stars. Major progress in coronal wave studies has been achieved thanks to the combination of high-precision multi-wavelength observations with spaceborne and ground-based facilities, elaborated theory of the interaction of MHD waves with plasma non-uniformities, state-of-the-art numerical simulations, and novel data analysis techniques. It has allowed the research community to reach a new look at the role played by MHD wave processes in the enigmatic phenomena of coronal plasma heating and wind acceleration as well as powerful energy releases such as flares and coronal mass ejections. In addition, the waves are intensively used as natural probes in the remote diagnostics of the coronal plasma parameters and physical processes operating in solar and stellar coronae via the method of MHD seismology. Individual chapters cover recent cutting-edge results obtained on the analysis and theoretical modelling of several most intensively studied coronal MHD wave phenomena, namely, kink and sausage oscillations of coronal loops and other field-aligned plasma structures, plus running and standing slow magnetoacoustic waves. A dedicated chapter assesses the reliability of proposed theoretical mechanisms for heating of the coronal plasma by MHD waves. Another chapter summarizes the current state of our understanding of the physical mechanisms and observational properties of quasi-periodic pulsations in solar flares, considers their analogy with similar processes detected in stellar flares, and thus establishes solid ground for the further exploitation of the solar-stellar analogy. An important discussion of novel data analysis techniques designed recently for MHD seismology applications is presented in a devoted chapter. The direction of future advances in the designated research areas are discussed.The book is a spin-off from the Topical Collection "Oscillatory Processes in Solar and Stellar Coronae" of the journal Space Science Reviews. Individual chapters cover recent cutting-edge results obtained on the analysis and theoretical modelling of several most intensively studied coronal MHD wave phenomena, namely, kink and sausage oscillations of coronal loops and other field-aligned plasma structures, plus running and standing slow magnetoacoustic waves. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.
Verlag: Amer Geophysical Union, 2016
ISBN 10: 1119054958ISBN 13: 9781119054955
Anbieter: GreatBookPrices, Columbia, MD, USA
Buch
Zustand: New.
Verlag: Amer Geophysical Union, 2016
ISBN 10: 1119054958ISBN 13: 9781119054955
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Zustand: As New. Unread book in perfect condition.
Verlag: Amer Geophysical Union, 2016
ISBN 10: 1119054958ISBN 13: 9781119054955
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
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Zustand: New. In.
Verlag: John Wiley & Sons 2016-04-12, 2016
ISBN 10: 1119054958ISBN 13: 9781119054955
Anbieter: Chiron Media, Wallingford, Vereinigtes Königreich
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Hardcover. Zustand: New.
Verlag: John Wiley & Sons, 2016
ISBN 10: 1119054958ISBN 13: 9781119054955
Anbieter: moluna, Greven, Deutschland
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Gebunden. Zustand: New. Low-frequency waves in space plasmas have been studied for several decades, and our knowledge gain has been incremental with several paradigm-changing leaps forward. In our solar system, such waves occur in the ionospheres and magnetospheres of planets, and.
Verlag: Amer Geophysical Union, 2016
ISBN 10: 1119054958ISBN 13: 9781119054955
Anbieter: Revaluation Books, Exeter, Vereinigtes Königreich
Buch
Hardcover. Zustand: Brand New. 1st edition. 528 pages. 11.50x9.00x1.00 inches. In Stock.
Verlag: Wiley-VCH, 2012
ISBN 10: 3527409947ISBN 13: 9783527409945
Anbieter: dsmbooks, Liverpool, Vereinigtes Königreich
Buch
Hardcover. Zustand: New. New. book.