New millennium solar physics (Record no. 560679)
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000 -LEADER | |
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fixed length control field | 02076 a2200229 4500 |
005 - DATE AND TIME OF LATEST TRANSACTION | |
control field | 20190826152936.0 |
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION | |
fixed length control field | 190822b xxu||||| |||| 00| 0 eng d |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
ISBN | 9783030139544 |
040 ## - CATALOGING SOURCE | |
Transcribing agency | IIT Kanpur |
041 ## - LANGUAGE CODE | |
Language code of text/sound track or separate title | eng |
082 ## - DEWEY DECIMAL CLASSIFICATION NUMBER | |
Classification number | 551.5 |
Item number | As23n |
100 ## - MAIN ENTRY--AUTHOR NAME | |
Personal name | Aschwanden, Markus J. |
245 ## - TITLE STATEMENT | |
Title | New millennium solar physics |
Statement of responsibility, etc | Markus J. Aschwanden |
260 ## - PUBLICATION, DISTRIBUTION, ETC. (IMPRINT) | |
Name of publisher | Springer |
Year of publication | 2019 |
Place of publication | Switzerland |
300 ## - PHYSICAL DESCRIPTION | |
Number of Pages | xv, 714p |
440 ## - SERIES STATEMENT/ADDED ENTRY--TITLE | |
Title | Astrophysics and space science library |
490 ## - SERIES STATEMENT | |
Series statement | / edited by Steven N. Shore ; v.458 |
520 ## - SUMMARY, ETC. | |
Summary, etc | This is a follow-on book to the introductory textbook "Physics of the Solar Corona" previously published in 2004 by the same author, which provided a systematic introduction and covered mostly scientific results from the pre-2000 era. Using a similar structure as the previous book the second volume provides a seamless continuation of numerous novel research results in solar physics that emerged in the new millennium (after 2000) from the new solar missions of RHESSI, STEREO, Hinode, CORONAS, and the Solar Dynamics Observatory (SDO) during the era of 2000-2018. The new solar space missions are characterized by unprecedented high-resolution imaging, time resolution, spectral capabilities, stereoscopy and tomography, which reveal the intricate dynamics of magneto-hydrodynamic processes in the solar corona down to scales of 100 km. The enormous amount of data streaming down from SDO in Terabytes per day requires advanced automated data processing methods. The book focuses exclusively on new research results after 2000, which are reviewed in a comprehensive manner, documented by over 3600 literature references, covering theory, observations, and numerical modeling of basic physical processes that are observed in high-temperature plasmas of the Sun and other astrophysical objects, such as plasma instabilities, coronal heating, magnetic reconnection processes, coronal mass ejections, plasma waves and oscillations, or particle acceleration. |
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM | |
Topical Term | Solar system |
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM | |
Topical Term | Astrophysics |
942 ## - ADDED ENTRY ELEMENTS (KOHA) | |
Koha item type | Books |
Withdrawn status | Lost status | Damaged status | Not for loan | Collection code | Permanent Location | Current Location | Date acquired | Source of acquisition | Cost, normal purchase price | Full call number | Accession Number | Cost, replacement price | Koha item type |
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General Stacks | PK Kelkar Library, IIT Kanpur | PK Kelkar Library, IIT Kanpur | 2019-09-02 | 2 | 8863.05 | 551.5 As23n | A184643 | 11078.81 | Books |