太平间 发表于 2025-3-21 19:19:20

书目名称Experimental and Theoretical Advances in Fluid Dynamics影响因子(影响力)<br>        http://figure.impactfactor.cn/if/?ISSN=BK0318981<br><br>        <br><br>书目名称Experimental and Theoretical Advances in Fluid Dynamics影响因子(影响力)学科排名<br>        http://figure.impactfactor.cn/ifr/?ISSN=BK0318981<br><br>        <br><br>书目名称Experimental and Theoretical Advances in Fluid Dynamics网络公开度<br>        http://figure.impactfactor.cn/at/?ISSN=BK0318981<br><br>        <br><br>书目名称Experimental and Theoretical Advances in Fluid Dynamics网络公开度学科排名<br>        http://figure.impactfactor.cn/atr/?ISSN=BK0318981<br><br>        <br><br>书目名称Experimental and Theoretical Advances in Fluid Dynamics被引频次<br>        http://figure.impactfactor.cn/tc/?ISSN=BK0318981<br><br>        <br><br>书目名称Experimental and Theoretical Advances in Fluid Dynamics被引频次学科排名<br>        http://figure.impactfactor.cn/tcr/?ISSN=BK0318981<br><br>        <br><br>书目名称Experimental and Theoretical Advances in Fluid Dynamics年度引用<br>        http://figure.impactfactor.cn/ii/?ISSN=BK0318981<br><br>        <br><br>书目名称Experimental and Theoretical Advances in Fluid Dynamics年度引用学科排名<br>        http://figure.impactfactor.cn/iir/?ISSN=BK0318981<br><br>        <br><br>书目名称Experimental and Theoretical Advances in Fluid Dynamics读者反馈<br>        http://figure.impactfactor.cn/5y/?ISSN=BK0318981<br><br>        <br><br>书目名称Experimental and Theoretical Advances in Fluid Dynamics读者反馈学科排名<br>        http://figure.impactfactor.cn/5yr/?ISSN=BK0318981<br><br>        <br><br>

sundowning 发表于 2025-3-21 21:52:33

Sky Dancer: A Complex Fluid-Structure Interactione to complex dynamics. Air flow which passes through the tube deforms the tube wall which in turn modifies the flow hydrodynamical properties, and so on. We present in this article an experiment which models a sky dancer. The blown air speed can be varied and tubes of low rigidity and of different d

insurrection 发表于 2025-3-22 01:39:14

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转换 发表于 2025-3-22 07:35:56

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诙谐 发表于 2025-3-22 12:36:34

Formation of Massive Stars by Runaway Accretionly because of the lack of a good observational guidance. One major conceptual problem in massive star formation arises from the radiation pressure they exert on the surrounding dust and gas, which could be strong enough to halt further accretion and impose a limit to the mass of a star. Radiation hy

duplicate 发表于 2025-3-22 15:02:13

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duplicate 发表于 2025-3-22 20:35:22

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Flatus 发表于 2025-3-22 21:57:04

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insincerity 发表于 2025-3-23 05:07:07

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不愿 发表于 2025-3-23 06:35:29

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查看完整版本: Titlebook: Experimental and Theoretical Advances in Fluid Dynamics; Jaime Klapp,Anne Cros,Mario Alberto Rodriguez Meza Book 2012 The Editor(s) (if ap