Electron and Proton Kinetics and Dynamics in Flaring Atmospheres PDF Download
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Author: Valentina Zharkova
Publisher: John Wiley & Sons
ISBN: 3527639675
Category : Science
Languages : en
Pages : 415
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Book Description
This timely book presents new research results on high-energy particle physics related to solar flares, covering the theory and applications of the reconnection process in a clear and comprehensible way. It investigates particle kinetics and dynamics in flaring atmospheres and their diagnostics from spectral observations, while providing an analysis of the observation data and techniques and comparing various models. Written by an internationally acclaimed expert, this is vital reading for all solar, astro-, and plasma physicists working in the field.
Author: Valentina Zharkova
Publisher: John Wiley & Sons
ISBN: 3527639675
Category : Science
Languages : en
Pages : 415
Get Book Here
Book Description
This timely book presents new research results on high-energy particle physics related to solar flares, covering the theory and applications of the reconnection process in a clear and comprehensible way. It investigates particle kinetics and dynamics in flaring atmospheres and their diagnostics from spectral observations, while providing an analysis of the observation data and techniques and comparing various models. Written by an internationally acclaimed expert, this is vital reading for all solar, astro-, and plasma physicists working in the field.
Author: Leonty Miroshnichenko
Publisher: Springer
ISBN: 3319094297
Category : Science
Languages : en
Pages : 533
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Book Description
Presents a comprehensive approach to the open questions in solar cosmic ray research and includes consistent and detailed considerations of conceptual, observational, theoretical, experimental and applied aspects of the field. The results of solar cosmic ray (SCR) investigations from 1942 to the present are summarized in this book. It treats the research questions in a self-contained form in all of its associations, from fundamental astrophysical aspects to geophysical, aeronautical and cosmonautical applications. A large amount of new data is included, which has been accumulated during the last several decades of space research. This second edition contains numerous updates and corrections to the text, figures and references. The author has also added several new sections about GLEs and radiation hazards. In addition, an extensive bibliography is provided, which covers non-partially the main achievements and failures in the field. This volume is aimed at graduate students and researchers in solar physics and space science.
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Category : Aeronautics
Languages : en
Pages : 1056
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Book Description
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Category : Dissertations, Academic
Languages : en
Pages : 348
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Category : Nuclear energy
Languages : en
Pages : 658
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Book Description
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Category : Physics
Languages : en
Pages : 1058
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Book Description
Author: Defense Documentation Center (U.S.)
Publisher:
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Category : Science
Languages : en
Pages : 1032
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Category : Aeronautics
Languages : en
Pages : 1148
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Book Description
Author: Gérard Trottet
Publisher:
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Category : Heliosphere
Languages : en
Pages : 246
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Book Description
Author: Vanessa Polito
Publisher: Frontiers Media SA
ISBN: 2832539335
Category : Science
Languages : en
Pages : 197
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Book Description
Since its launch in 2013, IRIS has observed more than 10 X-class, over 100 M-class and more than 600 C-class flares at unprecedented spatial and temporal resolution. Thanks to the rich diagnostics that cover the physical conditions of the solar atmosphere from the photosphere to the hottest parts of the flaring corona, IRIS observations have provided exciting new results and constraints on flare heating models, significantly expanding our knowledge of how flares are triggered, and how the non-thermal energy is released, propagates downward from the corona, and is deposited in the low atmosphere. At the same time, the new discoveries provided by IRIS have raised new unresolved questions and new challenges for theoretical models. For instance, current hydrodynamic models still cannot fully explain many features observed by IRIS during both the impulsive and gradual phases such as the dynamics of the evaporative/condensation flows, the large line broadenings, and the puzzling complex and broad chromospheric lines. In addition, important questions remain regarding the details of the energy propagation and dissipation in flares, the importance of Alfvén waves vs electron-beam and thermal conduction heating, and the effects from large-scale reconfiguration of the magnetic field during flares.
