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New millennium solar physics (Record no. 560679)

000 -LEADER
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
Holdings
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
        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

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