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Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere
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(Buch) |
Dieser Artikel gilt, aufgrund seiner Grösse, beim Versand als 3 Artikel!
Lieferstatus: |
Auf Bestellung (Lieferzeit unbekannt) |
Veröffentlichung: |
August 2019
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Genre: |
Naturwissensch., Medizin, Technik |
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Astronomy, Cosmology and Space Sciences /
B /
Complex systems /
Computer modelling & simulation /
computer science /
Computer simulation /
Data-driven Science, Modeling and Theory Building /
Earth and Environmental Science /
Ecological science, the Biosphere /
Econophysics /
Mathematical physics /
Numerical and Computational Physics, Simulation /
Physics /
Simulation and Modeling /
Social research & statistics /
Sociophysics /
Solar and Heliospheric Physics /
solar system /
Theoretical, Mathematical and Computational Physics |
ISBN: |
9789811390807 |
EAN-Code:
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9789811390807 |
Verlag: |
Springer Nature EN |
Einband: |
Gebunden |
Sprache: |
English
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Serie: |
Atmosphere, Earth, Ocean & Space |
Dimensionen: |
H 235 mm / B 155 mm / D |
Gewicht: |
1346 gr |
Seiten: |
772 |
Illustration: |
XIX, 772 p. 199 illus., 141 illus. in color., schwarz-weiss Illustrationen, farbige Illustrationen |
Bewertung: |
Titel bewerten / Meinung schreiben
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Inhalt: |
The book covers intimately all the topics necessary for the development of a robust magnetohydrodynamic (MHD) code within the framework of the cell-centered finite volume method (FVM) and its applications in space weather study. First, it presents a brief review of existing MHD models in studying solar corona and the heliosphere. Then it introduces the cell-centered FVM in three-dimensional computational domain. Finally, the book presents some applications of FVM to the MHD codes on spherical coordinates in various research fields of space weather, focusing on the development of the 3D Solar-InterPlanetary space-time Conservation Element and Solution Element (SIP-CESE) MHD model and its applications to space weather studies in various aspects. The book is written for senior undergraduates, graduate students, lecturers, engineers and researchers in solar-terrestrial physics, space weather theory, modeling, and prediction, computational fluid dynamics, and MHD simulations. It helps readers to fully understand and implement a robust and versatile MHD code based on the cell-centered FVM. |
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