Solar Energetic Particles A Modern Primer on Understanding Sources, Acceleration and Propagation /

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 dist...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Κύριος συγγραφέας: Reames, Donald V. (Συγγραφέας)
Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
Γλώσσα:English
Έκδοση: Cham : Springer International Publishing : Imprint: Springer, 2017.
Σειρά:Lecture Notes in Physics, 932
Θέματα:
Διαθέσιμο Online:Full Text via HEAL-Link
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245 1 0 |a Solar Energetic Particles  |h [electronic resource] :  |b A Modern Primer on Understanding Sources, Acceleration and Propagation /  |c by Donald V. Reames. 
264 1 |a Cham :  |b Springer International Publishing :  |b Imprint: Springer,  |c 2017. 
300 |a XVI, 127 p. 79 illus., 61 illus. in color.  |b online resource. 
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490 1 |a Lecture Notes in Physics,  |x 0075-8450 ;  |v 932 
505 0 |a Introduction -- History -- Distinguishing Two Sources -- Impulsive SEP events -- Gradual SEP Events -- High Energies and Radiation Effects -- Measurements of SEPs -- Summary and Conclusions. 
520 |a 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. 
650 0 |a Physics. 
650 0 |a Geophysics. 
650 0 |a Observations, Astronomical. 
650 0 |a Astronomy  |x Observations. 
650 0 |a Plasma (Ionized gases). 
650 1 4 |a Physics. 
650 2 4 |a Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). 
650 2 4 |a Plasma Physics. 
650 2 4 |a Geophysics/Geodesy. 
650 2 4 |a Astronomy, Observations and Techniques. 
710 2 |a SpringerLink (Online service) 
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776 0 8 |i Printed edition:  |z 9783319508702 
830 0 |a Lecture Notes in Physics,  |x 0075-8450 ;  |v 932 
856 4 0 |u http://dx.doi.org/10.1007/978-3-319-50871-9  |z Full Text via HEAL-Link 
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