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978-1-4614-1710-1Springer-Verlag New York 2009
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The Origin and Dynamics of Solar Magnetism978-1-4419-0239-9Series ISSN 1385-7525
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1385-7525 ity and thermal diffusivity that is far too large in comparison to magnetic diffusivity. Because of these discrepancies, the success of geodynamo models may seem surprising. In order to better understand978-1-4614-1710-1978-1-4419-0239-9Series ISSN 1385-7525
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Book 20091st editionow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many respects: they are dominated by the axial dipole of approximately the right strength, they show spatial power spectra similar to that of Earth, and the magnetic eld morphology and the temporal var- tion of
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发表于 2025-3-23 02:39:38
1385-7525 olar activity are treated in a very comprehensive wayStarting in 1995 numerical modeling of the Earth’s dynamo has ourished with remarkable success. Direct numerical simulation of convection-driven MHD- ow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many res
angiography
发表于 2025-3-23 07:59:03
A. R. Felthous M.D.,H. Sassent of methods of factoring which can, be used on these machines. Recent examples of spetacular factorizations include.where all factors on the right hand side are primes and . denotes a prime of . decimal digits.