New Millennium Solar Physics / / by Markus J. Aschwanden

• Record Nr.: UNINA9910337881803321
• Autore: Aschwanden Markus J
• Pubbl/distr/stampa: Cham : , : Springer International Publishing : , : Imprint : Springer, , 2019
• ISBN: 3-030-13956-5
• Edizione: [1st ed. 2019.]
• Descrizione fisica: 1 online resource (719 pages)
• Collana: Astrophysics and Space Science Library, , 0067-0057 ; ; 458
• Disciplina: 551.5; 523.7
• Soggetti: Solar system; Astrophysics; Observations, Astronomical; Astronomy—Observations; Space sciences; Solar and Heliospheric Physics; Astrophysics and Astroparticles; Astronomy, Observations and Techniques; Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)
• Lingua di pubblicazione: Inglese
• Formato: Materiale a stampa
• Livello bibliografico: Monografia
• Nota di contenuto: New 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.
• Sommario/riassunto: 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. .