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Titlebook: Eingangspostbearbeitung in Bürokommunikationssystemen; Expertensystemansatz Matthias Schumann Book 1987 Springer-Verlag Berlin Heidelberg 1

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發(fā)表于 2025-3-26 22:48:33 | 只看該作者
32#
發(fā)表于 2025-3-27 03:52:55 | 只看該作者
33#
發(fā)表于 2025-3-27 06:49:56 | 只看該作者
34#
發(fā)表于 2025-3-27 12:49:22 | 只看該作者
35#
發(fā)表于 2025-3-27 13:53:36 | 只看該作者
Vector-Parasite Interactions in Mosquito-Borne Filariasis,s a heritable trait, but genes that control susceptibility have not yet been identified. Likewise, nothing is known about gene expression in filarial worms as it relates to adaptation of the parasite to the mosquito host environment. Mosquitoes are equipped with several means to prevent the establis
36#
發(fā)表于 2025-3-27 19:21:51 | 只看該作者
Book 1979ernational Perimetric Society. The Proceedings of this symposium follow the general lines of the pro- gramme with some minor alterations. This symposium was a so-called topic-symposium where selected topics were introduced by experts in the field. These topics were: Neuro-ophtha[mo[ogy. 1. Funduscop
37#
發(fā)表于 2025-3-27 22:47:46 | 只看該作者
38#
發(fā)表于 2025-3-28 04:41:03 | 只看該作者
Mathematical Model of Particle Swarm Optimization: Numerical Optimization Problemsspark the interest of the reader. Readers wishing to learn more about the applications of PSO and its variants to multi-objective, constrained, dynamic optimization problems and other advanced topics are recommended to consider the various references at the end of the chapter.
39#
發(fā)表于 2025-3-28 09:01:41 | 只看該作者
SAT Heritage: A Community-Driven Effort for Archiving, Building and Running More Than Thousand SAT Solvers,tools for archiving and building binaries (thanks to Docker, GitHub and Zenodo) and provide a consistent and easy way for this. Thanks to our tool, building (or running) a solver from its source (or from its binary) can be done in one line.
40#
發(fā)表于 2025-3-28 11:02:05 | 只看該作者
G. A. Bazilevskaya,I. G. Usoskin,E. O. Flückiger,R. G. Harrison,L. Desorgher,R. Bütikofer,M. B. Krainev,V. S. Makhmutov,Y. I. Stozhkov,A. K. Svirzhevskaya,N. S. Svirzhevsky,G. A. Kovaltsov surface (f-) mode solutions are also discussed. While not attempting to be comprehensive, it is hoped that the summary presented in this chapter addresses the most important theoretical aspects that are required for a solid start in stellar pulsations research.
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