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001430971 001__ 1430971
001430971 003__ OCoLC
001430971 005__ 20230308003215.0
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001430971 008__ 210324s2021\\\\sz\a\\\\ob\\\\000\0\eng\d
001430971 019__ $$a1244629674
001430971 020__ $$a9783030664022$$q(electronic bk.)
001430971 020__ $$a3030664023$$q(electronic bk.)
001430971 020__ $$z9783030664015$$q(print)
001430971 0247_ $$a10.1007/978-3-030-66402-2$$2doi
001430971 035__ $$aSP(OCoLC)1243073639
001430971 040__ $$aGW5XE$$beng$$erda$$epn$$cGW5XE$$dOCLCO$$dSFB$$dEBLCP$$dOCLCF$$dOCLCQ$$dUKAHL$$dOCLCO$$dCOM$$dOCLCQ
001430971 049__ $$aISEA
001430971 050_4 $$aQB526.S65
001430971 08204 $$a536.7/223$$223
001430971 1001_ $$aReames, Donald V.,$$eauthor.
001430971 24510 $$aSolar energetic particles :$$ba modern primer on understanding sources, acceleration and propagation /$$cDonald V. Reames.
001430971 250__ $$aSecond edition.
001430971 264_1 $$aCham, Switzerland :$$bSpringer,$$c2021.
001430971 300__ $$a1 online resource (xvi, 225 pages) :$$billustrations (some color)
001430971 336__ $$atext$$btxt$$2rdacontent
001430971 337__ $$acomputer$$bc$$2rdamedia
001430971 338__ $$aonline resource$$bcr$$2rdacarrier
001430971 4901_ $$aLecture notes in physics,$$x0075-8450 ;$$vvolume 978
001430971 504__ $$aIncludes bibliographical references.
001430971 5050_ $$aPreface -- Introducing the Sun and SEPs -- A Turbulent History -- Distinguishing the Sources -- Impulsive SEP Events -- Gradual SEP Events -- High Energies and Radiation Effects -- Measurements of SEPs -- Elemental Abundances and FIP: SEPs, The Corona and the Solar Wind -- Hydrogen Abundances and Shock Waves -- Summary and Conclusions.
001430971 5060_ $$aOpen access.$$5GW5XE
001430971 520__ $$aThis 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.
001430971 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed March 24, 2021).
001430971 650_0 $$aSolar energetic particles.
001430971 650_6 $$aParticules énergétiques solaires.
001430971 655_0 $$aElectronic books.
001430971 7760_ $$z3030664015
001430971 830_0 $$aLecture notes in physics ;$$v978.$$x0075-8450
001430971 852__ $$bebk
001430971 85640 $$3Springer Nature$$uhttps://link.springer.com/10.1007/978-3-030-66402-2$$zOnline Access$$91397441.2
001430971 909CO $$ooai:library.usi.edu:1430971$$pGLOBAL_SET
001430971 980__ $$aBIB
001430971 980__ $$aEBOOK
001430971 982__ $$aEbook
001430971 983__ $$aOnline
001430971 994__ $$a92$$bISE