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Titlebook: Solar Dynamics and Magnetism from the Interior to the Atmosphere; Nagi N. Mansour,Alexander G. Kosovichev,Dana Longc Book 2014 Springer Sc

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Variability of Solar Five-Minute Oscillations in the Corona as Observed by the , (ESP) on the , (SD spectra for a 49-day period of low and intermediate solar activity showed little correlation with the mean EUV irradiance and the short-term variability of the irradiance. We suggest that some other changes in the solar atmosphere, ., magnetic fields and/or inter-network configuration may affect th
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,A Comparison of Solar Cycle Variations in the Equatorial Rotation Rates of the Sun’s Subsurface, Suation in the yearly mean equatorial-rotation rate of the sunspot groups seems to be lagging behind that of the equatorial-rotation rate determined from the GONG measurements by one to two years. The amplitude of the GONG measurements is very small. The solar-cycle variation in the equatorial-rotatio
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Comparing Simulations of Rising Flux Tubes Through the Solar Convection Zone with Observations of Sles about the Joy’s Law trend, the most commonly occurring tilt angle, the rotation rate of the emerging loops with respect to the surrounding plasma, and the nature of the magnetic field at the flux tube apex. We discuss how these diagnostic properties constrain the initial field strength of the ac
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The Sub-surface Structure of a Large Sample of Active Regions,e find that the magnitudes of these perturbations depend on the strength of the surface magnetic field, but we find a great deal of scatter in this relation, implying that other factors may be relevant.
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Horizontal Flows in the Photosphere and Subphotosphere of Two Active Regions,hin the sunspot penumbra. The area having inward flows in the subphotosphere is larger than that in the photosphere. For AR 11158, flows in these two layers show great similarities in some areas and significant differences in other areas. Both layers exhibit consistent outward flows in the areas sur
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Book 2014magnetic activity at various spatial and temporal scales. This book demonstrates that the synergy of high-resolution multi-wavelength observations and simulations is a key to uncovering the long-standing puzzles of solar magnetism and dynamics..This volume is aimed at researchers and graduate studen
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Douglas Goughn strong and weak racial states (Goldberg 2005). Strong racial states exist where racial divisions and exclusions are the result of explicit commitment and where they are a routine feature of governance, public policy and administration. The example of the Israeli state and its pursuit of racial Pal
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