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Solar Energetic Particles: A Modern Primer on Understanding Sources, Acceleratio
US $80,43
CircaEUR 69,06
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Spedizione:
Gratis USPS Media MailTM.
Oggetto che si trova a: 20772, Stati Uniti
Consegna:
Consegna prevista tra il sab 18 ott e il mar 21 ott a 94104
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Restituzioni entro 30 giorni. Le spese di spedizione del reso sono a carico dell'acquirente..
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Numero oggetto eBay:146243422966
Specifiche dell'oggetto
- Condizione
- ISBN
- 9783319508702
Informazioni su questo prodotto
Product Identifiers
Publisher
Springer International Publishing A&G
ISBN-10
3319508709
ISBN-13
9783319508702
eBay Product ID (ePID)
236688654
Product Key Features
Book Title
Solar Energetic Particles : a Modern Primer on Understanding Sources, Acceleration and Propagation
Number of Pages
Xvi, 127 Pages
Language
English
Topic
Physics / Geophysics, Physics / Astrophysics, Power Resources / Alternative & Renewable, Physics / Nuclear
Publication Year
2017
Illustrator
Yes
Genre
Technology & Engineering, Science
Book Series
Lecture Notes in Physics Ser.
Format
Trade Paperback
Dimensions
Item Weight
80.8 Oz
Item Length
9.3 in
Item Width
6.1 in
Additional Product Features
Dewey Edition
23
Series Volume Number
932
Number of Volumes
1 vol.
Dewey Decimal
523.72
Table Of Content
Introduction.- History.- Distinguishing Two Sources.- Impulsive SEP events.- Gradual SEP Events.- High Energies and Radiation Effects.- Measurements of SEPs.- Summary and Conclusions.
Synopsis
This concise primer introduces the non-specialist reader to the physics of solar energetic particles (SEP) and systematically reviews the evidence for the two main mechanisms which lead to the so-called impulsive and gradual SEP events. More specifically, the timing of the onsets, the longitude distributions, the high-energy spectral shapes, the correlations with other solar phenomena (e.g. coronal mass ejections), as well as the all-important elemental and isotopic abundances of SEPs are investigated. Impulsive SEP events are related 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 new technique to determine the source plasma temperature in both impulsive and gradual events is demonstrated. Last but not least the role of SEP events as a radiation hazard in space is mentioned and a short discussion of the nature of the main particle telescope designs that have contributed to most of the SEP measurements is given., This concise primer introduces the non-specialist reader to the physics of solar energetic particles (SEP) and systematically reviews the evidence for the two main mechanisms which lead to the so-called impulsive and gradual SEP events. More specifically, the timing of the onsets, the longitude distributions, the high-energy spectral shapes, the correlations with other solar phenomena (e.g. coronal mass ejections), as well as the all-important elemental and isotopic abundances of SEPs are investigated. Impulsive SEP events are related to magnetic reconnection in solar flares and jets. The concept of shock acceleration by scattering on self-amplified Alfv n 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 new technique to determine the source plasma temperature in both impulsive and gradual events is demonstrated. Last but not least the role of SEP events as a radiation hazard in space is mentioned and a short discussion of the nature of the main particle telescope designs that have contributed to most of the SEP measurements is given.
LC Classification Number
QC1-75
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