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New millennium solar physics

Aschwanden, Markus J.

New millennium solar physics

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	New millennium solar physicsby Markus J. Aschwanden.
作者:	Aschwanden, Markus J.
出版者:	Cham :Springer International Publishing :2019.
面頁冊數:	xv, 714 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
標題:	Solar activity.
標題:	Sun.
電子資源:	https://doi.org/10.1007/978-3-030-13956-8
ISBN:	9783030139568$q(electronic bk.)

New millennium solar physics
Aschwanden, Markus J.

New millennium solar physics[electronic resource] /by Markus J. Aschwanden. - Cham :Springer International Publishing :2019. - xv, 714 p. :ill., digital ;24 cm. - Astrophysics and space science library,v.4580067-0057 ;. - Astrophysics and space science library ;379..

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.

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.

ISBN: 9783030139568$q(electronic bk.)

Standard No.: 10.1007/978-3-030-13956-8doiSubjects--Topical Terms:

276016
Solar activity.
Subjects--Geographical Terms:

283395
Sun.

LC Class. No.: QB521 / .A834 2019

Dewey Class. No.: 523.7

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520 $a 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.
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