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一氧化碳分子(CO)在星际空间中的丰度仅次于氢气(H2)分子，排在第二位。CO吸收宇宙空间中的真空紫外辐射以后会解离生成C原子和O原子；碎片原子会进一步和H2分子反应生成碳氢化合物和水，而这些次生分子是组成生命的基本物质。另一方面，CO的光吸收和光解离还被认为是造成太阳系中C、O同位素异常分布的直接原因，从分子层面理解这一现象形成的机制对于研究太阳系的演化历史以及行星的形成机制具有重要的意义。
CFD Simulation of the Flow around NREL Phase VI Wind Turbine
CFD Simulation NREL Phase VI Wind Turbine
2014/10/23
The simulation of the turbulent and potentially separating flow around a rotating, twisted, and tapered airfoil is a challenging task for CFD simulations. This thesis describes CFD simulations of the ...
The driving goal of Natural Resource Ecology Laboratory science is to increase the fundamental understanding of our environment, through collaborative application of ecology and ecosystem science prin...
March 06, 2007，Two scientists at the U.S. Department of Energy's National Renewable Energy Laboratory have been named Dan David Prize Laureates for 2007. Jerry Olson and Sarah Kurtz will receive their...