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  • 1
    Online Resource
    Online Resource
    Dordrecht : Springer Netherlands
    UID:
    b3kat_BV045178924
    Format: 1 Online-Ressource (VIII, 228 p)
    ISBN: 9789401725415
    Content: Over the last decade we entered a new exploration phase of solar flare physics, equipped with powerful spacecraft such as Yohkoh, SoHO, and TRACE that pro vide us detail-rich and high-resolution images of solar flares in soft X-rays, hard X -rays, and extreme-ultraviolet wavelengths. Moreover, the large-area and high sensitivity detectors on the Compton GRO spacecraft recorded an unprecedented number of high-energy photons from solar flares that surpasses all detected high energy sources taken together from the rest of the universe, for which CGRO was mainly designed to explore. However, morphological descriptions of these beau tiful pictures and statistical catalogs of these huge archives of solar data would not convey us much understanding of the underlying physics, if we would not set out to quantify physical parameters from these data and would not subject these measurements to theoretical models. Historically, there has always been an unsatisfactory gap between traditional astronomy that dutifully describes the mor phology of observations, and the newer approach of astrophysics, which starts with physical concepts from first principles and analyzes astronomical data with the goal to confirm or disprove theoretical models. In this review we attempt to bridge this yawning gap and aim to present the recent developments in solar flare high-energy physics from a physical point of view, structuring the observations and analysis results according to physical processes, such as particle acceleration, propagation, energy loss, kinematics, and radiation signatures
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 9789048160624
    Language: English
    URL: Volltext  (URL des Erstveröffentlichers)
    URL: Volltext  (lizenzpflichtig)
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  • 2
    Book
    Book
    Berlin : Springer
    UID:
    gbv_390315605
    Format: XXI, 842 S , Ill., graph. Darst , 242 mm x 170 mm
    ISBN: 3540223215
    Series Statement: Springer-Praxis books in geophysical sciences
    Note: Literaturverz. S. [757] - 818
    Language: English
    Subjects: Physics
    RVK:
    Keywords: Sonnenkorona ; Physik
    URL: Cover
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  • 3
    UID:
    kobvindex_ZLB15267327
    Format: XIV, 420 Seiten , Ill., graph. Darst.
    Edition: 1
    ISBN: 9783642150005
    Note: Text engl.
    Language: English
    Keywords: Astrophysik ; Nichtlineare Dynamik ; Selbst organisierendes System ; Kritisches Phänomen
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  • 4
    UID:
    b3kat_BV036491224
    Format: 1 Online-Ressource
    Edition: Reprint. with corr., problems and solutions
    ISBN: 9783540307662
    Series Statement: Springer-Praxis books in astronomy and planetary sciences
    Additional Edition: Erscheint auch als Druckausgabe ISBN 978-3-540-30765-5
    Language: English
    Subjects: Physics
    RVK:
    Keywords: Sonnenkorona ; Physik
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  • 5
    Book
    Book
    Berlin [u.a.] : Springer-Verlag
    UID:
    kobvindex_ZLB13974551
    Format: XVII, 892 Seiten , Ill., graph. Darst. , 25 cm
    Edition: Repr.
    ISBN: 3540307656
    Series Statement: Springer Praxis books in astronomy and planetary sciences
    Note: Text engl.
    Language: English
    Keywords: Sonnenkorona ; Physik
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  • 6
    UID:
    almahu_9949198565202882
    Format: XIII, 388 p. , online resource.
    Edition: 1st ed. 2003.
    ISBN: 9789400710634
    Series Statement: NATO Science Series II: Mathematics, Physics and Chemistry, Mathematics, Physics and Chemistry ; 124
    Content: Significant advances have been made recently in both the theoretical understanding and observation of small-scale turbulence in different layers of the Sun, and in the instabilities that give rise to them. The general development of solar physics, however, has led to such a degree of specialization as to hinder interaction between workers in the field. This book therefore presents studies of different layers and regions of the Sun, but from the same aspect, concentrating on the study of small-scale motions. The main emphasis is on the common theoretical roots of these phenomena, but the book also contains an extensive treatment of the observational aspects.
    Note: One / Instabilities and Motions in the Solar Interior and Tachocline -- A dynamo in the radiative interior -- Turbulence and its Sources Below the Convective Zone -- MHD simulations of small and large scale dynamos -- Two / Turbulence in the Convective Zone and Photosphere -- Helioseismic observations of plasma motions in the solar convection zone -- Turbulent Transport in Rotating and Magnetized Fluids -- Three / Parker Instability and Flux Tube Dynamics -- Three-dimensional Evolution of a Magnetic Flux Tube Emerging into the Solar Atmosphere -- Photospheric magnetic field at small scales -- Four / Waves and Oscillations in the Solar Atmosphere -- Waves in the chromosphere: observations -- Theory of MHD Waves in the Solar Corona -- Prominence Oscillations: Theory -- Review of Coronal Oscillations - An Observer's View -- Nonlinear Waves in the Magnetically Structured Solar Atmosphere -- Five / Turbulence and Reconnection in the Solar Corona -- TRACE and Ground-based Observations of Small-scale Dynamics in Active Regions -- Observational Signatures of Magnetic Reconnection -- Self-organized Structures in the Solar Atmosphere: Theory and Observations -- Six / Solar Wind -- Wave Heating and Acceleration of the Fast Solar Wind -- Waves and turbulence in the solar wind.
    In: Springer Nature eBook
    Additional Edition: Printed edition: ISBN 9781402016592
    Additional Edition: Printed edition: ISBN 9781402016585
    Additional Edition: Printed edition: ISBN 9789400710641
    Language: English
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  • 7
    Online Resource
    Online Resource
    Dordrecht :Springer Netherlands :
    UID:
    almahu_9948601374902882
    Format: VIII, 228 p. , online resource.
    Edition: 1st ed. 2002.
    ISBN: 9789401725415
    Content: Over the last decade we entered a new exploration phase of solar flare physics, equipped with powerful spacecraft such as Yohkoh, SoHO, and TRACE that pro­ vide us detail-rich and high-resolution images of solar flares in soft X-rays, hard X -rays, and extreme-ultraviolet wavelengths. Moreover, the large-area and high­ sensitivity detectors on the Compton GRO spacecraft recorded an unprecedented number of high-energy photons from solar flares that surpasses all detected high­ energy sources taken together from the rest of the universe, for which CGRO was mainly designed to explore. However, morphological descriptions of these beau­ tiful pictures and statistical catalogs of these huge archives of solar data would not convey us much understanding of the underlying physics, if we would not set out to quantify physical parameters from these data and would not subject these measurements to theoretical models. Historically, there has always been an unsatisfactory gap between traditional astronomy that dutifully describes the mor­ phology of observations, and the newer approach of astrophysics, which starts with physical concepts from first principles and analyzes astronomical data with the goal to confirm or disprove theoretical models. In this review we attempt to bridge this yawning gap and aim to present the recent developments in solar flare high-energy physics from a physical point of view, structuring the observations and analysis results according to physical processes, such as particle acceleration, propagation, energy loss, kinematics, and radiation signatures.
    Note: From the contents: 1: Introduction -- 2: Magnetic Topology of Acceleration Regions -- 3: Geometry of Acceleration Regions -- 4: Dynamics of Acceleration Region -- 5: Accelerating Electromagnetic Fields and Waves -- 6: Particle Kinematics. 7: Gamma Ray Emission -- 8: Hard X-Ray Emission -- 9: Radio Emission -- 10: Conclusions -- References.
    In: Springer Nature eBook
    Additional Edition: Printed edition: ISBN 9789048160624
    Additional Edition: Printed edition: ISBN 9781402007255
    Additional Edition: Printed edition: ISBN 9789401725422
    Language: English
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  • 8
    Online Resource
    Online Resource
    Berlin, Heidelberg :Springer Berlin Heidelberg :
    UID:
    almahu_9949195266802882
    Format: XXII, 908 p. , online resource.
    Edition: 1st ed. 2005.
    ISBN: 9783540307662
    Series Statement: Astronomy and Planetary Sciences,
    Content: Solar science has evolved rapidly over the past ten years as the results of a new generation of solar space missions have become available. This book provides a thorough introduction to the subject of solar physics, based on those spacecraft observations. The author introduces the solar corona, which has a temperature of several million degrees, and sets it in the context of basic plasma physics before moving on to discuss plasma instabilities and plasma heating processes. The latest results on coronal heating and radiation,which are fundamental processes in all stars, are presented. Spectacular phenomena such as solar flares and coronal mass ejections are described in detail, together with their potential effects on the Earth. The author draws together observations made at many wavelengths from hard X-rays, soft X-rays, extreme UV and radio wavelengths. This paperback study edition of Markus Aschwanden's highly acclaimed PHYSICS OF THE SOLAR CORONA will include 50 pages of problems and solutions which will much enhance the value of the book to students.
    Note: Thermal Radiation -- Hydrostatics -- Hydrodynamics -- Magnetic Fields -- Magneto-Hydrodynamics (MHD) -- MHD Oscillations -- Propagating MHD Waves -- Coronal Heating -- Magnetic Reconnection -- Particle Acceleration -- Particle Kinematics -- Hard X-Rays -- Gamma-Rays -- Radio Emission -- Flare Plasma Dynamics -- Coronal Mass Ejections (CMEs).
    In: Springer Nature eBook
    Additional Edition: Printed edition: ISBN 9783540818533
    Additional Edition: Printed edition: ISBN 9783540860389
    Additional Edition: Printed edition: ISBN 9783540307655
    Additional Edition: Printed edition: ISBN 9783540223214
    Language: English
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  • 9
    Book
    Book
    Berlin : Springer | Chichester, UK : Praxis Publ.
    UID:
    gbv_505538164
    Format: XXII, 892 S , zahlr. Ill. und graph. Darst , 25 cm
    Edition: Reprint. with corr., problems and solutions
    ISBN: 9783540307655 , 3540307656
    Series Statement: Springer Praxis books in astronomy and planetary sciences
    Note: Literaturverz. S. 807 - 868
    Additional Edition: Erscheint auch als Online-Ausgabe Aschwanden, Markus J. Physics of the Solar Corona Berlin, Heidelberg : Praxis Publishing Ltd, Chichester, UK, 2005 ISBN 9783540307662
    Language: English
    Subjects: Physics
    RVK:
    Keywords: Sonnenkorona ; Physik
    URL: Cover
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  • 10
    Online Resource
    Online Resource
    Cham : Springer
    UID:
    gbv_166672839X
    Format: 1 Online-Ressource (XV, 714 Seiten) , Illustrationen, Diagramme
    ISBN: 9783030139568
    Series Statement: Astrophysics and Space Science Library 458
    Content: New Solar Instrumentation -- Atomic Physics and Spectroscopy -- The Solar Interior -- The Photosphere and Sunspots -- The Chromosphere and Spicules -- The Quiet Sun Corona -- Coronal Holes and Jets -- Active Regions -- Coronal Loops -- Coronal Loop Oscillation and Waves -- Filaments and Prominences -- Flares: Nonthermal Particles -- Flares: Thermal Emission -- CME Initiation -- CME Propagation -- Sun-Earth Connections
    Content: This is a follow-on book to the introductory textbook "Physics of the Solar Corona" previously published in 2004 by the same author, which provided a systematic introduction and covered mostly scientific results from the pre-2000 era. Using a similar structure as the previous book the second volume provides a seamless continuation of numerous novel research results in solar physics that emerged in the new millennium (after 2000) from the new solar missions of RHESSI, STEREO, Hinode, CORONAS, and the Solar Dynamics Observatory (SDO) during the era of 2000-2018. The new solar space missions are characterized by unprecedented high-resolution imaging, time resolution, spectral capabilities, stereoscopy and tomography, which reveal the intricate dynamics of magneto-hydrodynamic processes in the solar corona down to scales of 100 km. The enormous amount of data streaming down from SDO in Terabytes per day requires advanced automated data processing methods. The book focuses exclusively on new research results after 2000, which are reviewed in a comprehensive manner, documented by over 3600 literature references, covering theory, observations, and numerical modeling of basic physical processes that are observed in high-temperature plasmas of the Sun and other astrophysical objects, such as plasma instabilities, coronal heating, magnetic reconnection processes, coronal mass ejections, plasma waves and oscillations, or particle acceleration
    Additional Edition: ISBN 9783030139551
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 978-3-030-13955-1
    Language: English
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