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Titlebook: Water Snowline in Protoplanetary Disks; Shota Notsu Book 2020 The Editor(s) (if applicable) and The Author(s), under exclusive license to

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樓主: SORB
31#
發(fā)表于 2025-3-26 23:47:25 | 只看該作者
iately take up the arising challenges. For crucial gaps in current concepts we sketch solutions and explain implications on user-controlled identity management systems. Finally we give recommendations to stakeholders such as data controllers, application designers and policy makers.
32#
發(fā)表于 2025-3-27 03:59:40 | 只看該作者
Shota Notsuptimization algorithms in the literature. More specifically, for anonymization algorithms that process datasets in column-wise order, we show that a random column ordering can lead to significantly higher quality solutions than orderings determined by known greedy heuristics.
33#
發(fā)表于 2025-3-27 08:29:14 | 只看該作者
34#
發(fā)表于 2025-3-27 13:18:07 | 只看該作者
Shota Notsuerungsversuchs Schorndorfs soll zur Illustration der Situation in Baden-Württemberg im folgenden dargestellt werden. Im Anschlu? daran wird am Beispiel der Stadt Friedrichshafen die grunds?tzliche Problematik einer Privatisierung der Abwasserbeseitigung diskutiert.
35#
發(fā)表于 2025-3-27 16:15:07 | 只看該作者
at any point during runtime, ascertains the dynamic selection of the component with the optimal anticipated personalization effects among those that are permissible under the currently prevailing privacy constraints.
36#
發(fā)表于 2025-3-27 19:30:24 | 只看該作者
37#
發(fā)表于 2025-3-28 01:18:24 | 只看該作者
38#
發(fā)表于 2025-3-28 02:23:01 | 只看該作者
39#
發(fā)表于 2025-3-28 08:50:51 | 只看該作者
Modeling Studies III. Sub-millimeter H, ,O and H, ,O Lines,ses, the local intensity from the outer optically thin region in the disk is around . times smaller than that in the infrared candidate water line cases. Therefore, in the sub-millimeter lines, especially H. .O and para-H. .O lines with relatively lower upper state energies (.a few 100?K) can also l
40#
發(fā)表于 2025-3-28 11:34:55 | 只看該作者
Modeling Studies III. Sub-millimeter H, ,O and H, ,O Lines,ses, the local intensity from the outer optically thin region in the disk is around . times smaller than that in the infrared candidate water line cases. Therefore, in the sub-millimeter lines, especially H. .O and para-H. .O lines with relatively lower upper state energies (.a few 100?K) can also l
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