Titlebook: Helioseismic Diagnostics of Solar Convection and Activity; Thomas L. Duvall,John W. Harvey,Zdeněk Švestka Book 2001 Springer Science+Busin

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C. Lindsey,D. C. Braunutiful and well-grounded applications which connect broadly to many areas of mathematics. We of course hope that students will pursue this material independently; teachers may find it useful for undergraduate seminars. For an overview of the material presented, consult the table of contents and the

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D. C. Braun,C. Lindsey mathematicians (and very many practitioners) must have the skills to work with convex sets and functions, and extremal problems, since convexity continually crops up in the investigation of very diverse problems in mathematics and the natural sciences. It seems that some of the elements of convex a

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Fluid Dynamics and MHD of the Solar Convection Zone and Tachocline: Current Understanding and Unsolvnetic structures; global convection and circulation; the rise of magnetic flux tubes to the photosphere, and their injection into the base of the convection zone; tachocline fluid dynamics and MHD; and the solar dynamo. We close with a set of observational’ targets’ for helioseismologists to aim for

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The Coupling of Solar Convection and Rotation (Invited Review) tremendous advances in high-performance computing technology, prompting increasingly sophisticated and realistic numerical models of solar convection. Among the most important helioseismic constraints on global-scale convection models is the mean differential rotation profile of the solar envelope,

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Realistic Solar Convection Simulationsate and radiative energy exchange. The simulation results are compared quantitatively with observations. Excellent agreement is obtained for the distribution of the emergent continuum intensity, the profiles of weak photospheric lines, the .mode frequencies, the asymmetrical shape of the mode veloci

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