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Titlebook: Maximum Entropy and Bayesian Methods Garching, Germany 1998; Proceedings of the 1 Wolfgang Linden,Volker Dose,Roland Preuss Conference proc

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樓主: Coagulant
21#
發(fā)表于 2025-3-25 04:37:15 | 只看該作者
22#
發(fā)表于 2025-3-25 07:54:13 | 只看該作者
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發(fā)表于 2025-3-25 12:34:14 | 只看該作者
Do Kestern occurrence 388 10. 1. 5 Summary 391 10. 2 Kelvin-Helmholtz Instability at the Flank Magnetopause 391 10. 3 Microphysics of Magnetopause Processes 396 10. 3. 1978-94-007-8909-8978-1-4020-4582-0Series ISSN 1385-7525
24#
發(fā)表于 2025-3-25 19:02:06 | 只看該作者
G. Larry Bretthorst to the dust evaporation temperature. Dynamical e ects due to tidal interaction of the binary system are supposed to be responsible for pushing the disk inner radius outwards..The spectrum of AK Sco exhibits emission and absorption lines that show substantial variety and variability in shape. The sy
25#
發(fā)表于 2025-3-25 20:05:47 | 只看該作者
26#
發(fā)表于 2025-3-26 03:05:00 | 只看該作者
27#
發(fā)表于 2025-3-26 07:38:54 | 只看該作者
N. Rivier,B. Dubertret,T. Aste,H. Ohlenbuschere is no one set of flux products that represents the best possible choice for GODAE in all regions and all components is adopted. An alternative merger of a variety of different datasets is described along with objective corrections based on regional and/or short term observations, and ocean model
28#
發(fā)表于 2025-3-26 09:18:50 | 只看該作者
29#
發(fā)表于 2025-3-26 15:22:37 | 只看該作者
V. Vengrinovich,Yu. Denkevich,G.-R. Tillackndamental ways as well, driven by the complexity of the instruments used and their tremendous cost. The conclusion of this paper is that optical/infrared ground-based astronomy is in transition. “Hundred-million-dollar-scale” 8m to 10m telescopes have been erected and now our communities have billio
30#
發(fā)表于 2025-3-26 17:22:54 | 只看該作者
E. Fischer,W. Jacob,W. Von Der Linden,V. Dose 1. 2 Component vs. anti-parallel reconnection 382 10. 1. 3 Tailward-of-the-cusp reconnection 385 10. 1. 4 Quantitative tests of reconnection occurrence 388 10. 1. 5 Summary 391 10. 2 Kelvin-Helmholtz Instability at the Flank Magnetopause 391 10. 3 Microphysics of Magnetopause Processes 396 10. 3. 1
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