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Titlebook: Challenges to Theories of the Structure of Moderate-Mass Stars; Proceedings of a Con Douglas Gough,Juri Toomre Conference proceedings 1991

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21#
發(fā)表于 2025-3-25 04:41:54 | 只看該作者
Antimicrobial Functions of Neutrophils,distribution of the spacings violates the Poisson distribution, which should hold under conditions of spherical symmetry of the equilibrium state of the sun. The relevance of this result in connection with inversion problems is briefly emphasised.
22#
發(fā)表于 2025-3-25 10:03:06 | 只看該作者
23#
發(fā)表于 2025-3-25 12:36:23 | 只看該作者
Lecture Notes in Earth Sciencesiate density contrast. The general flow patterns consist of a series of rolls in the horizontal which are coherent throughout the entire vertical domain, much like findings by a number of investigators. The horizontal component of the subgrid-scale (SGS) force appears to enhance fluctuations of pres
24#
發(fā)表于 2025-3-25 19:01:10 | 只看該作者
25#
發(fā)表于 2025-3-25 22:02:21 | 只看該作者
Phanerozoic Phosphorite Depositional Systemsanalyzed to determine the spectrum of the solar supergranulation. Individual Dopplergrams were averaged together using a weighted average over 20-minute intervals to remove the p-mode oscillations. The Doppler signals due to the motion of the observer, the solar rotation, differential rotation, and
26#
發(fā)表于 2025-3-26 03:57:38 | 只看該作者
Phosphate minerals and sediments,ayer. The convective flows are found to consist of rolls which are coherent throughout the entire vertical domain, similar to the results of a number of earlier investigations. Motions near the upper boundary are supersonic, though the Rayleigh number is moderate. The major effect of a high density
27#
發(fā)表于 2025-3-26 05:33:08 | 只看該作者
Challenges to Theories of the Structure of Moderate-Mass Stars978-3-540-38355-0Series ISSN 0075-8450 Series E-ISSN 1616-6361
28#
發(fā)表于 2025-3-26 11:19:42 | 只看該作者
B. Trierweiler-Hauke,J. Busch M.A.olar outer layers by as much as 20% in the standard models. However the necessity of explaining also the lithium destruction in the sun and solar type stars reduces the expected helium depletion to a few percent.
29#
發(fā)表于 2025-3-26 16:01:27 | 只看該作者
30#
發(fā)表于 2025-3-26 17:30:16 | 只看該作者
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