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000780302 019__ $$a984860565
000780302 020__ $$a9783319508719$$q(electronic book)
000780302 020__ $$a3319508717$$q(electronic book)
000780302 020__ $$z9783319508702
000780302 0247_ $$a10.1007/978-3-319-50871-9$$2doi
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000780302 035__ $$aSP(OCoLC)977680827$$z(OCoLC)984860565
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000780302 049__ $$aISEA
000780302 050_4 $$aQB526.S65
000780302 08204 $$a536.7/223$$223
000780302 1001_ $$aReames, D. V.,$$eauthor.
000780302 24510 $$aSolar energetic particles :$$ba modern primer on understanding sources, acceleration and propagation /$$cDonald V. Reames.
000780302 264_1 $$aCham, Switzerland :$$bSpringer,$$c2017.
000780302 300__ $$a1 online resource (xvi, 127 pages) :$$billustrations.
000780302 336__ $$atext$$btxt$$2rdacontent
000780302 337__ $$acomputer$$bc$$2rdamedia
000780302 338__ $$aonline resource$$bcr$$2rdacarrier
000780302 347__ $$atext file$$bPDF$$2rda
000780302 4901_ $$aLecture notes in physics,$$x0075-8450 ;$$vvolume 932
000780302 504__ $$aIncludes bibliographical references.
000780302 5050_ $$aIntroduction -- History -- Distinguishing Two Sources -- Impulsive SEP events -- Gradual SEP Events -- High Energies and Radiation Effects -- Measurements of SEPs -- Summary and Conclusions.
000780302 506__ $$aAccess limited to authorized users.
000780302 520__ $$aThis concise primer introduces the non-specialist reader to the physics of solar energetic particles (SEP) and systematically reviews the evidence for the two main mechanisms which lead to the so-called impulsive and gradual SEP events. More specifically, the timing of the onsets, the longitude distributions, the high-energy spectral shapes, the correlations with other solar phenomena (e.g. coronal mass ejections), as well as the all-important elemental and isotopic abundances of SEPs are investigated. Impulsive SEP events are related to magnetic reconnection in solar flares and jets. The concept of shock acceleration by scattering on self-amplified Alfvén waves is introduced, as is the evidence of reacceleration of impulsive-SEP material in the seed population accessed by the shocks in gradual events. The text then develops processes of transport of ions out to an observer. Finally, a new technique to determine the source plasma temperature in both impulsive and gradual events is demonstrated. Last but not least the role of SEP events as a radiation hazard in space is mentioned and a short discussion of the nature of the main particle telescope designs that have contributed to most of the SEP measurements is given.
000780302 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed March 21, 2017).
000780302 650_0 $$aSolar energetic particles.
000780302 77608 $$iPrint version:$$z9783319508702
000780302 830_0 $$aLecture notes in physics ;$$v932.
000780302 852__ $$bebk
000780302 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-3-319-50871-9$$zOnline Access$$91397441.1
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000780302 980__ $$aEBOOK
000780302 980__ $$aBIB
000780302 982__ $$aEbook
000780302 983__ $$aOnline
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