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Titlebook: Zerst?rungsfreie Prüfverfahren; Radiografie und Radi Dieter Stegemann Book 1995 Springer Fachmedien Wiesbaden 1995 Computer.Fertigung.Forsc

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樓主: 武士精神
21#
發(fā)表于 2025-3-25 04:23:30 | 只看該作者
22#
發(fā)表于 2025-3-25 07:35:58 | 只看該作者
Compression Models from Elementary Incremental Lawsnd void ratio. Models were presented in terms of void ratio-effective stress relationship and porosity-depth trends. All theoretical expressions were derived by assuming suitable incremental compression laws. Comparison with experimental data indicates that the models can describe a number of featur
23#
發(fā)表于 2025-3-25 12:09:37 | 只看該作者
24#
發(fā)表于 2025-3-25 18:19:40 | 只看該作者
Meeting at the Midway: Systems, Partnerships and Collaborative Inquiry to Generate Practice Based Evidence, families, and societies. Science has also shown us prevention is possible. With growing evidence that child maltreatment prevention programs can be effective, a current challenge lies in getting communities to take up these strategies and allocate resources to “upstream” prevention efforts. Taking
25#
發(fā)表于 2025-3-25 21:25:39 | 只看該作者
Motivating Software Engineers Working in Virtual Teams Across the Globesoftware engineer is to ‘identify with their task’ which requires being given a task that is challenging and understanding the purpose and significance of the task in relation to the complete system being developed. Software engineers’ needs are complex – they also require regular feedback, trust, a
26#
發(fā)表于 2025-3-26 00:20:30 | 只看該作者
27#
發(fā)表于 2025-3-26 05:06:15 | 只看該作者
Synthetic Images of Proto-Planetary Disks Around Young Stars,egions; (2) the scattering of stellar photons in the optically thin parts of the disk; and (3) the thermal emission of the disk due to viscous energy dissipation during the accretion process. We discuss the relative importance of these emission processes at wavelengths ranging from 1.2 to 20 μm.
28#
發(fā)表于 2025-3-26 11:36:04 | 只看該作者
29#
發(fā)表于 2025-3-26 14:17:27 | 只看該作者
30#
發(fā)表于 2025-3-26 17:11:59 | 只看該作者
Sarah Garcia,Denis Laesker,Derek Caprio,Ronald Kauer,Jason Nguyen,Marvin Andujar processing method for fuzzy star maps and distortion correction method for star maps, providing high-quality star maps for star map matching. Second, an effective star map identification method is introduced to acquire effective starlight vector direction. Finally, a star sensor-based celestial nav
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