000 06220nam a2200685 i 4500
001 9780750322324
003 IOP
005 20220908114311.0
006 m eo d
007 cr cn |||m|||a
008 200106s2020 enka ob 000 0 eng d
020 _a9780750322324
_qebook
020 _a9780750322317
_qmobi
020 _z9780750322300
_qprint
020 _z9780750322331
_qmyPrint
024 7 _a10.1088/2514-3433/ab404a
_2doi
035 _a(CaBNVSL)thg00979911
035 _a(OCoLC)1135509952
040 _aCaBNVSL
_beng
_erda
_cCaBNVSL
_dCaBNVSL
050 4 _aQB524
_b.M594 2020eb
072 7 _aPGS
_2bicssc
072 7 _aSCI004000
_2bisacsh
082 0 4 _a523.7/5 $223
100 1 _aMiyake, Fusa,
_eauthor.
_934733
245 1 0 _aExtreme solar particle storms :
_bthe hostile Sun /
_cFusa Miyake, Ilya Usoskin and Stepan Poluianov.
246 3 0 _aHostile Sun.
264 1 _aBristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) :
_bIOP Publishing,
_c[2020]
300 _a1 online resource (various pagings) :
_billustrations (some color).
336 _atext
_2rdacontent
337 _aelectronic
_2isbdmedia
338 _aonline resource
_2rdacarrier
490 1 _aAAS-IOP astronomy. [release 2],
_x2514-3433
500 _a"Version: 20191201"--Title page verso.
504 _aIncludes bibliographical references.
505 0 _a1. Introduction -- 2. What can be learned from modern data? -- 2.1. Strength of solar flares -- 2.2. Solar particle events -- 2.3. Major geomagnetic storms
505 8 _a3. State-of-the-art theory and modeling -- 3.1. Solar and stellar dynamos -- 3.2. Particle acceleration at the sun
505 8 _a4. Cosmogenic isotopes as proxies for solar energetic particles -- 4.1. What can we learn about SPEs in the past? -- 4.2. Production of cosmogenic isotopes in the atmosphere -- 4.3. Isotope transport -- 4.4. Isotope archiving in ice cores -- 4.5. Lunar archives
505 8 _a5. Measurements of radionuclides -- 5.1. Measurement techniques -- 5.2. Tree rings -- 5.3. Analysis of cosmogenic isotopes recorded in ice cores
505 8 _a6. Characterization of the measured events -- 6.1. Observed SEP events: knowns and unknowns -- 6.2. Reconstruction of energy spectra -- 6.3. Known visual auroral observations -- 6.4. Event statistics and the worst-case scenario
505 8 _a7. Further search for extreme events -- 7.1. Terrestrial cosmogenic isotopes -- 7.2. Historical archival records -- 7.3. Sun-like stars
505 8 _a8. Possible impacts -- 8.1. Environmental effects -- 8.2. Technological and societal effects -- 9. Concluding remarks.
520 3 _aIt is becoming increasingly clear that our modern technological society is vulnerable to the impacts of severe solar storms, radiation, particle and geomagnetic disturbances. However, the potential severity of these extreme solar events and their probability of occurring are unknown. What can we expect from the Sun? What could the most severe solar particle storms look like? Does the Sun have an unlimited ability to produce severe storms? Can a destructive "black swan" event occur? Direct solar data covers only several decades, a period too short to answer these questions. Fortunately, other indirect ways to study these possibly rare extreme solar storms have been discovered, paving the way for analysis of these events on the multi-millennial time scale. At present, studies of extreme solar events are growing, forming a new research discipline. This book, written by leaders in the corresponding aspects of the field, presents a first systematic review of the current state of the art.
521 _aMSc/PhD level students in Space Physics; researchers in Space Sciences and Astrophysics; Environmental researchers.
530 _aAlso available in print.
538 _aMode of access: World Wide Web.
538 _aSystem requirements: Adobe Acrobat Reader, EPUB reader, or Kindle reader.
545 _aFusa Miyake was educated at the Division of Particle and Astrophysical Science, Nagoya University. She obtained her PhD at Nagoya University in 2013, and has since worked for the Institute for Advanced Research and Solar-Terrestrial Environment Laboratory (now Institute for Space-Earth Environmental Research), Nagoya University. She, together with a team of researchers, discovered the extreme solar events of 775 CE and 993 CE in the cosmogenic isotope (initially in 14C), that formed the field of this book. Ilya Usoskin is a full professor in Space Physics at the University of Oulu and has worked as the head of Oulu Cosmic Ray Station since 2000. He is also the vice-director of ReSoLVE (Research on SOlar Long-term Variability and Effects) Center of Excellence of the Academy of Finland. Ilya received his Cand.Sci degree from the A.F. Ioffe Physical-Technical Institute and his PhD from the University of Oulu. His awards include the knighthood (1st class knight) of the Order of the Lion of Finland (2013), Julis Bartels medal (2018) of the European Geosciences Union, and membership in the Finnish Academy of Sciences and Letters. Stepan Poluianov got his degree at the ITMO (Information Technologies, Mechanics and Optics) University in St. Petersburg. He worked at the Polar Geophysical Institute before earning his PhD in Space Physics at the University Oulu, Finland. Stepan continues to work at the University of Oulu, studying cosmic rays and their interaction with matter. In 2019, he became a member of the AMS collaboration that runs the cosmic ray experiment AMS-02 at the International Space Station.
588 0 _aTitle from PDF title page (viewed on January 6, 2020).
650 0 _aSolar activity.
_919624
650 0 _aSolar activity
_xForecasting.
_937846
650 7 _aSolar system - the Sun & planets.
_2bicssc
_937820
650 7 _aSCIENCE / Astronomy.
_2bisacsh
700 1 _aUsoskin, Ilya G.,
_eauthor.
_934735
700 1 _aPoluianov, Stepan,
_eauthor.
_934734
710 2 _aInstitute of Physics (Great Britain),
_epublisher.
776 0 8 _iPrint version:
_z9780750322300
_z9780750322331
830 0 _aAAS-IOP astronomy.
_pRelease 2.
856 4 0 _uhttps://iopscience.iop.org/book/978-0-7503-2232-4
942 _cEBK
999 _c57516
_d57516