LEADER 04301nam 22006135 450 001 9910337881803321 005 20200702220958.0 010 $a3-030-13956-5 024 7 $a10.1007/978-3-030-13956-8 035 $a(CKB)4100000008280573 035 $a(MiAaPQ)EBC5780017 035 $a(DE-He213)978-3-030-13956-8 035 $a(PPN)236522329 035 $a(EXLCZ)994100000008280573 100 $a20190522d2019 u| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aNew Millennium Solar Physics /$fby Markus J. Aschwanden 205 $a1st ed. 2019. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2019. 215 $a1 online resource (719 pages) 225 1 $aAstrophysics and Space Science Library,$x0067-0057 ;$v458 311 $a3-030-13954-9 327 $aNew Solar Instrumentation -- Atomic Physics and Spectroscopy -- The Solar Interior -- The Photosphere and Sunspots -- The Chromosphere and Spicules -- The Quiet Sun Corona -- Coronal Holes and Jets -- Active Regions -- Coronal Loops -- Coronal Loop Oscillation and Waves -- Filaments and Prominences -- Flares: Nonthermal Particles -- Flares: Thermal Emission -- CME Initiation -- CME Propagation -- Sun-Earth Connections. 330 $aThis is a follow-on book to the introductory textbook "Physics of the Solar Corona" previously published in 2004 by the same author, which provided a systematic introduction and covered mostly scientific results from the pre-2000 era. Using a similar structure as the previous book the second volume provides a seamless continuation of numerous novel research results in solar physics that emerged in the new millennium (after 2000) from the new solar missions of RHESSI, STEREO, Hinode, CORONAS, and the Solar Dynamics Observatory (SDO) during the era of 2000-2018. The new solar space missions are characterized by unprecedented high-resolution imaging, time resolution, spectral capabilities, stereoscopy and tomography, which reveal the intricate dynamics of magneto-hydrodynamic processes in the solar corona down to scales of 100 km. The enormous amount of data streaming down from SDO in Terabytes per day requires advanced automated data processing methods. The book focuses exclusively on new research results after 2000, which are reviewed in a comprehensive manner, documented by over 3600 literature references, covering theory, observations, and numerical modeling of basic physical processes that are observed in high-temperature plasmas of the Sun and other astrophysical objects, such as plasma instabilities, coronal heating, magnetic reconnection processes, coronal mass ejections, plasma waves and oscillations, or particle acceleration. . 410 0$aAstrophysics and Space Science Library,$x0067-0057 ;$v458 606 $aSolar system 606 $aAstrophysics 606 $aObservations, Astronomical 606 $aAstronomy?Observations 606 $aSpace sciences 606 $aSolar and Heliospheric Physics $3https://scigraph.springernature.com/ontologies/product-market-codes/P22070 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 606 $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030 615 0$aSolar system. 615 0$aAstrophysics. 615 0$aObservations, Astronomical. 615 0$aAstronomy?Observations. 615 0$aSpace sciences. 615 14$aSolar and Heliospheric Physics . 615 24$aAstrophysics and Astroparticles. 615 24$aAstronomy, Observations and Techniques. 615 24$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). 676 $a551.5 676 $a523.7 700 $aAschwanden$b Markus J$4aut$4http://id.loc.gov/vocabulary/relators/aut$01063071 906 $aBOOK 912 $a9910337881803321 996 $aNew Millennium Solar Physics$92529929 997 $aUNINA