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OverviewMagnetohydrodynamics describes dynamics in electrically conductive fluids. These occur in our environment as well as in our atmosphere and magnetosphere, and play a role in the sun's interaction with our planet. In most cases these phenomena involve turbulences, and thus are very challenging to understand and calculate. A sound knowledge is needed to tackle these problems. This work gives the basic information on turbulence in nature, comtaining the needed equations, notions and numerical simulations. The current state of our knowledge and future implications of MHD turbulence are outlined systematically. It is indispensable for all scientists engaged in research of our atmosphere and in space science. Full Product DetailsAuthor: Andrey Beresnyak , Alexander LazarianPublisher: De Gruyter Imprint: De Gruyter Edition: Digital original Volume: 12 Dimensions: Width: 17.00cm , Height: 1.80cm , Length: 24.00cm Weight: 0.611kg ISBN: 9783110262902ISBN 10: 3110262908 Pages: 286 Publication Date: 08 July 2019 Audience: Professional and scholarly , Professional & Vocational , Professional & Vocational Format: Hardback Publisher's Status: Active Availability: In stock  We have confirmation that this item is in stock with the supplier. It will be ordered in for you and dispatched immediately. Table of Contents1. MHD Turbulence Observed in nature 2. Basic Equations 3. Statistical and Numerical Methods 4. Incompressible MHD turbulence 5. Origin of the Magnetic Fields 6. Compressible MHD turbulenceReviewsAuthor InformationAndrey Beresnyak and Alexander Lazarian, Department of Astronomy, University of Wisconsin-Madison, USA. Tab Content 6Author Website:Countries AvailableAll regions |
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