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Verfasst von:Reames, Donald V. [VerfasserIn]   i
Titel:Solar Energetic Particles
Titelzusatz:A Modern Primer on Understanding Sources, Acceleration and Propagation
Verf.angabe:by Donald V. Reames
Ausgabe:2nd ed. 2021.
Verlagsort:Cham
 Cham
Verlag:Springer International Publishing
 Imprint: Springer
E-Jahr:2021
Jahr:2021.
 2021.
Umfang:1 Online-Ressource(XVI, 225 p. 124 illus., 103 illus. in color.)
Gesamttitel/Reihe:Lecture Notes in Physics ; 978
 Springer eBook Collection
Fussnoten:Open Access
ISBN:978-3-030-66402-2
Abstract:Preface -- Introducing the Sun and SEPs -- A Turbulent History -- Distinguishing the Sources -- Impulsive SEP Events -- Gradual SEP Events -- High Energies and Radiation Effects -- Measurements of SEPs -- Elemental Abundances and FIP: SEPs, The Corona and the Solar Wind -- Hydrogen Abundances and Shock Waves -- Summary and Conclusions.
 This open access book serves as a concise primer introducing the non-specialist reader to the physics of solar energetic particles (SEP). It systematically reviews the evidence for the two main mechanisms which lead to the so-called impulsive and gradual SEP events. This second edition contains two completely new chapters discussing element abundances and shock waves, reflecting new theoretical, modeling, and observational results. Existing chapters have been substantially expanded or updated with additions placed in a broader context. More specifically, the author discusses the timing of the onsets of SEPs, their longitude distributions, their high-energy spectral shapes, their correlations with other solar phenomena, as well as the all-important elemental and isotopic abundances. The book relates impulsive SEP events to magnetic reconnection in solar flares and jets. The concept of shock acceleration by scattering on self-amplified Alfvén waves is introduced, as is the evidence of reacceleration of impulsive-SEP material in the seed population accessed by the shocks in gradual events. The text then develops processes of transport of ions out to an observer. Finally, a technique to determine the source plasma temperature in both impulsive and gradual events is demonstrated.The author also mentions the role of SEP events as a radiation hazard in space and briefly discusses the nature of the main particle telescope designs that have contributed to most of the SEP measurements.
DOI:doi:10.1007/978-3-030-66402-2
URL:kostenfrei: Resolving-System: https://doi.org/10.1007/978-3-030-66402-2
 DOI: https://doi.org/10.1007/978-3-030-66402-2
Schlagwörter:(s)Energiereiches Teilchen   i / (g)Sonne   i
Datenträger:Online-Ressource
Sprache:eng
Bibliogr. Hinweis:Erscheint auch als : Druck-Ausgabe
 Erscheint auch als : Druck-Ausgabe
K10plus-PPN:1753065895
 
 
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