| 000 | 04645cam a2200757 i 4500 | ||
|---|---|---|---|
| 001 | ocn977680827 | ||
| 003 | OCoLC | ||
| 005 | 20250703114535.0 | ||
| 006 | m o d | ||
| 007 | cr cnu|||unuuu | ||
| 008 | 170321s2017 sz a ob 000 0 eng d | ||
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_a9783319508719 _q(electronic bk.) |
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| 020 |
_a3319508717 _q(electronic bk.) |
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| 020 | _a3319508709 | ||
| 020 | _a9783319508702 | ||
| 020 |
_a9783319508726 _q(print) |
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| 020 | _a3319508725 | ||
| 020 |
_z9783319508702 _q(print) |
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| 024 | 7 |
_a10.1007/978-3-319-50871-9 _2doi |
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_a(OCoLC)977680827 _z(OCoLC)984860565 _z(OCoLC)1005792752 _z(OCoLC)1011903556 _z(OCoLC)1014072689 _z(OCoLC)1021265995 _z(OCoLC)1066476512 _z(OCoLC)1086467640 _z(OCoLC)1111241640 _z(OCoLC)1112578377 |
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| 037 |
_acom.springer.onix.9783319508719 _bSpringer Nature |
||
| 050 | 4 | _aQB526.S65 | |
| 072 | 7 |
_aTTDS _2bicssc |
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| 072 | 7 |
_aTTDS _2thema |
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| 082 | 0 | 4 |
_a536.7/223 _223 |
| 049 | _aMAIN | ||
| 100 | 1 |
_aReames, D. V., _eauthor. _914433 |
|
| 245 | 1 | 0 |
_aSolar energetic particles : _ba modern primer on understanding sources, acceleration and propagation / _cDonald V. Reames. |
| 264 | 1 |
_aCham, Switzerland : _bSpringer, _c2017. |
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| 300 |
_a1 online resource (xvi, 127 pages) : _billustrations (some color) |
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| 336 |
_atext _btxt _2rdacontent |
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| 337 |
_acomputer _bc _2rdamedia |
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| 338 |
_aonline resource _bcr _2rdacarrier |
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| 347 |
_atext file _bPDF _2rda |
||
| 490 | 1 |
_aLecture notes in physics, _x0075-8450 ; _vvolume 932 |
|
| 504 | _aIncludes bibliographical references. | ||
| 588 | 0 | _aOnline resource; title from PDF title page (SpringerLink, viewed March 21, 2017). | |
| 505 | 0 | _aIntroduction -- History -- Distinguishing Two Sources -- Impulsive SEP events -- Gradual SEP Events -- High Energies and Radiation Effects -- Measurements of SEPs -- Summary and Conclusions. | |
| 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. | ||
| 650 | 0 |
_aSolar energetic particles. _98880 |
|
| 650 | 6 |
_aParticules énergétiques solaires. _9968733 |
|
| 650 | 7 |
_aPlasma physics. _2bicssc |
|
| 650 | 7 |
_aGeophysics. _2bicssc _98181 |
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| 650 | 7 |
_aAstronomy, space & time. _2bicssc _914363 |
|
| 650 | 7 |
_aAstronautics. _2bicssc |
|
| 650 | 7 |
_aScience _xNuclear Physics. _2bisacsh |
|
| 650 | 7 |
_aScience _xGeophysics. _2bisacsh _914304 |
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| 650 | 7 |
_aScience _xAstronomy. _2bisacsh _98844 |
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| 650 | 7 |
_aScience _xAstrophysics & Space Science. _2bisacsh |
|
| 650 | 7 |
_aSolar energetic particles _2fast _98880 |
|
| 655 | 7 |
_aObservations _2fast _913830 |
|
| 776 | 0 | 8 |
_iPrinted edition: _z9783319508702 |
| 830 | 0 |
_aLecture notes in physics ; _v932. _x0075-8450 |
|
| 856 | 4 | 0 | _uhttps://link-springer-com.libraryproxy.ist.ac.at/10.1007/978-3-319-50871-9 |
| 938 |
_aAskews and Holts Library Services _bASKH _nAH34381060 |
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| 938 |
_aProQuest Ebook Central _bEBLB _nEBL5596017 |
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