Extreme solar particle storms : (Record no. 57516)
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000 -LEADER | |
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fixed length control field | 06220nam a2200685 i 4500 |
001 - CONTROL NUMBER | |
control field | 9780750322324 |
003 - CONTROL NUMBER IDENTIFIER | |
control field | IOP |
005 - DATE AND TIME OF LATEST TRANSACTION | |
control field | 20220908114311.0 |
006 - FIXED-LENGTH DATA ELEMENTS--ADDITIONAL MATERIAL CHARACTERISTICS | |
fixed length control field | m eo d |
007 - PHYSICAL DESCRIPTION FIXED FIELD--GENERAL INFORMATION | |
fixed length control field | cr cn |||m|||a |
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION | |
fixed length control field | 200106s2020 enka ob 000 0 eng d |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
International Standard Book Number | 9780750322324 |
Qualifying information | ebook |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
International Standard Book Number | 9780750322317 |
Qualifying information | mobi |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
Canceled/invalid ISBN | 9780750322300 |
Qualifying information | |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
Canceled/invalid ISBN | 9780750322331 |
Qualifying information | myPrint |
024 7# - OTHER STANDARD IDENTIFIER | |
Standard number or code | 10.1088/2514-3433/ab404a |
Source of number or code | doi |
035 ## - SYSTEM CONTROL NUMBER | |
System control number | (CaBNVSL)thg00979911 |
035 ## - SYSTEM CONTROL NUMBER | |
System control number | (OCoLC)1135509952 |
040 ## - CATALOGING SOURCE | |
Original cataloging agency | CaBNVSL |
Language of cataloging | eng |
Description conventions | rda |
Transcribing agency | CaBNVSL |
Modifying agency | CaBNVSL |
050 #4 - LIBRARY OF CONGRESS CALL NUMBER | |
Classification number | QB524 |
Item number | .M594 2020eb |
072 #7 - SUBJECT CATEGORY CODE | |
Subject category code | PGS |
Source | bicssc |
072 #7 - SUBJECT CATEGORY CODE | |
Subject category code | SCI004000 |
Source | bisacsh |
082 04 - DEWEY DECIMAL CLASSIFICATION NUMBER | |
Classification number | 523.7/5 $223 |
100 1# - MAIN ENTRY--PERSONAL NAME | |
Personal name | Miyake, Fusa, |
Relator term | author. |
9 (RLIN) | 34733 |
245 10 - TITLE STATEMENT | |
Title | Extreme solar particle storms : |
Remainder of title | the hostile Sun / |
Statement of responsibility, etc. | Fusa Miyake, Ilya Usoskin and Stepan Poluianov. |
246 30 - VARYING FORM OF TITLE | |
Title proper/short title | Hostile Sun. |
264 #1 - PRODUCTION, PUBLICATION, DISTRIBUTION, MANUFACTURE, AND COPYRIGHT NOTICE | |
Place of production, publication, distribution, manufacture | Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) : |
Name of producer, publisher, distributor, manufacturer | IOP Publishing, |
Date of production, publication, distribution, manufacture, or copyright notice | [2020] |
300 ## - PHYSICAL DESCRIPTION | |
Extent | 1 online resource (various pagings) : |
Other physical details | illustrations (some color). |
336 ## - CONTENT TYPE | |
Content type term | text |
Source | rdacontent |
337 ## - MEDIA TYPE | |
Media type term | electronic |
Source | isbdmedia |
338 ## - CARRIER TYPE | |
Carrier type term | online resource |
Source | rdacarrier |
490 1# - SERIES STATEMENT | |
Series statement | AAS-IOP astronomy. [release 2], |
International Standard Serial Number | 2514-3433 |
500 ## - GENERAL NOTE | |
General note | "Version: 20191201"--Title page verso. |
504 ## - BIBLIOGRAPHY, ETC. NOTE | |
Bibliography, etc. note | Includes bibliographical references. |
505 0# - FORMATTED CONTENTS NOTE | |
Formatted contents note | 1. 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# - FORMATTED CONTENTS NOTE | |
Formatted contents note | 3. State-of-the-art theory and modeling -- 3.1. Solar and stellar dynamos -- 3.2. Particle acceleration at the sun |
505 8# - FORMATTED CONTENTS NOTE | |
Formatted contents note | 4. 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# - FORMATTED CONTENTS NOTE | |
Formatted contents note | 5. Measurements of radionuclides -- 5.1. Measurement techniques -- 5.2. Tree rings -- 5.3. Analysis of cosmogenic isotopes recorded in ice cores |
505 8# - FORMATTED CONTENTS NOTE | |
Formatted contents note | 6. 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# - FORMATTED CONTENTS NOTE | |
Formatted contents note | 7. Further search for extreme events -- 7.1. Terrestrial cosmogenic isotopes -- 7.2. Historical archival records -- 7.3. Sun-like stars |
505 8# - FORMATTED CONTENTS NOTE | |
Formatted contents note | 8. Possible impacts -- 8.1. Environmental effects -- 8.2. Technological and societal effects -- 9. Concluding remarks. |
520 3# - SUMMARY, ETC. | |
Summary, etc. | It 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 ## - TARGET AUDIENCE NOTE | |
Target audience note | MSc/PhD level students in Space Physics; researchers in Space Sciences and Astrophysics; Environmental researchers. |
530 ## - ADDITIONAL PHYSICAL FORM AVAILABLE NOTE | |
Additional physical form available note | Also available in print. |
538 ## - SYSTEM DETAILS NOTE | |
System details note | Mode of access: World Wide Web. |
538 ## - SYSTEM DETAILS NOTE | |
System details note | System requirements: Adobe Acrobat Reader, EPUB reader, or Kindle reader. |
545 ## - BIOGRAPHICAL OR HISTORICAL DATA | |
Biographical or historical data | Fusa 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# - SOURCE OF DESCRIPTION NOTE | |
Source of description note | Title from PDF title page (viewed on January 6, 2020). |
650 #0 - SUBJECT ADDED ENTRY--TOPICAL TERM | |
Topical term or geographic name entry element | Solar activity. |
9 (RLIN) | 19624 |
650 #0 - SUBJECT ADDED ENTRY--TOPICAL TERM | |
Topical term or geographic name entry element | Solar activity |
General subdivision | Forecasting. |
9 (RLIN) | 37846 |
650 #7 - SUBJECT ADDED ENTRY--TOPICAL TERM | |
Topical term or geographic name entry element | Solar system - the Sun & planets. |
Source of heading or term | bicssc |
9 (RLIN) | 37820 |
650 #7 - SUBJECT ADDED ENTRY--TOPICAL TERM | |
Topical term or geographic name entry element | SCIENCE / Astronomy. |
Source of heading or term | bisacsh |
700 1# - ADDED ENTRY--PERSONAL NAME | |
Personal name | Usoskin, Ilya G., |
Relator term | author. |
9 (RLIN) | 34735 |
700 1# - ADDED ENTRY--PERSONAL NAME | |
Personal name | Poluianov, Stepan, |
Relator term | author. |
9 (RLIN) | 34734 |
710 2# - ADDED ENTRY--CORPORATE NAME | |
Corporate name or jurisdiction name as entry element | Institute of Physics (Great Britain), |
Relator term | publisher. |
776 08 - ADDITIONAL PHYSICAL FORM ENTRY | |
Relationship information | Print version: |
International Standard Book Number | 9780750322300 |
-- | 9780750322331 |
830 #0 - SERIES ADDED ENTRY--UNIFORM TITLE | |
Uniform title | AAS-IOP astronomy. |
Name of part/section of a work | Release 2. |
856 40 - ELECTRONIC LOCATION AND ACCESS | |
Uniform Resource Identifier | <a href="https://iopscience.iop.org/book/978-0-7503-2232-4">https://iopscience.iop.org/book/978-0-7503-2232-4</a> |
942 ## - ADDED ENTRY ELEMENTS (KOHA) | |
Koha item type | E-Books |
No items available.