000			02076 a2200229 4500
005			20190826152936.0
008			190822b xxu||||| |||| 00| 0 eng d
020			_a9783030139544
040			_cIIT Kanpur
041			_aeng
082			_a551.5 _bAs23n
100			_aAschwanden, Markus J.
245			_aNew millennium solar physics _cMarkus J. Aschwanden
260			_bSpringer _c2019 _aSwitzerland
300			_axv, 714p
440			_aAstrophysics and space science library
490			_a/ edited by Steven N. Shore ; v.458
520			_aThis 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			_aSolar system
650			_aAstrophysics
942			_cBK
999			_c560679 _d560679