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频散效应对自由大气能量输送的影响 被引量:2
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作者 黄伟 刘式适 《北京大学学报(自然科学版)》 CAS CSCD 北大核心 1993年第5期595-603,共9页
本文应用扩大的Prandtl混合长理论分析自由大气中的Renolds平均运动方程组,着重分析了频散效应对自由大气大尺度运动能量输送的影响,分析指出:频散效应是自由大气中能量由扰动动能向平均动能转换(即能量逆转)的根本原因;正压大气能量逆... 本文应用扩大的Prandtl混合长理论分析自由大气中的Renolds平均运动方程组,着重分析了频散效应对自由大气大尺度运动能量输送的影响,分析指出:频散效应是自由大气中能量由扰动动能向平均动能转换(即能量逆转)的根本原因;正压大气能量逆转只能在扰动的尺度小于临界尺度Lc时才能发生;斜压大气能量逆转主要在扰动的厚度小于临界厚度Dc时发生。不同尺度的扰动与包含和不包含频散效应的简单模式结果验证了上面的结论。 展开更多
关键词 频散 能量逆转 自由大气
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Nonequilibrium Thermodynamics of Dark Energy on Cosmic Apparent Horizon 被引量:1
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作者 WANG Gang LIU Wen-Biao 《Communications in Theoretical Physics》 SCIE CAS CSCD 2009年第8期383-384,共2页
In recent several years,some works have been done on cosmic thermodynamics.The apparent horizonwas regarded as the key characteristic supersurface where thermodynamics can be built on perfectly.However,if theirreversi... In recent several years,some works have been done on cosmic thermodynamics.The apparent horizonwas regarded as the key characteristic supersurface where thermodynamics can be built on perfectly.However,if theirreversible process is considered,the proper position for building thermodynamics will not be the apparent horizonanymore.The new position is related to dark energy state equation and the irreversible process parameters. 展开更多
关键词 COSMOLOGY dark energy linear nonequilibrium thermodynamics ENTROPY apparent horizon
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不可压缩湍流的色散模型 被引量:1
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作者 董鹤 高歌 邸亚超 《航空动力学报》 EI CAS CSCD 北大核心 2013年第1期90-95,共6页
分析了广泛存在于湍流运动中的能量逆转现象,揭示了其产生的原因,提出了湍流的色散性质.在此基础上,修改了Boussinesq假设,建立了包含色散效应的新的雷诺应力封闭式和湍流色散系数,给出与不同模型相结合时,湍流色散系数所具有的不同形式... 分析了广泛存在于湍流运动中的能量逆转现象,揭示了其产生的原因,提出了湍流的色散性质.在此基础上,修改了Boussinesq假设,建立了包含色散效应的新的雷诺应力封闭式和湍流色散系数,给出与不同模型相结合时,湍流色散系数所具有的不同形式,并阐述了湍流运动中能量的传递方向及条件.采用不可压缩平板边界层流动和平面后台阶流动验证了其可信性和优越性.平板摩擦阻力系数及边界层速度型与实验结果吻合良好,平面后台阶流动的流向再附长度、台阶边压力系数及湍流强度等参数均比标准k-ε模型更接近实验结果.结果表明:色散项的加入可以在不显著增加计算量的同时显著改善预测精度,模型具有一定的工程应用价值. 展开更多
关键词 湍流 色散效应 涡黏模型 能量逆转 负黏性
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Feasibility analysis of the angular momentum reversal trajectory via hodograph method for high performance solar sails 被引量:3
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作者 ZENG XiangYuan BAOYIN HeXi +1 位作者 LI JunFeng GONG ShengPing 《Science China(Technological Sciences)》 SCIE EI CAS 2011年第11期2951-2957,共7页
In this paper a new phase space of hodograph method is adopted to investigate and better understand the two-dimensional angular momentum reversal(H-reversal) trajectories for high performance solar sails within a fixe... In this paper a new phase space of hodograph method is adopted to investigate and better understand the two-dimensional angular momentum reversal(H-reversal) trajectories for high performance solar sails within a fixed cone angle.As the hodograph method and the H-reversal trajectory are not very common,both of them are briefly introduced.The relationship between them are constructed and addressed with a sample trajectory.How the phase space varies according to the sail quality and the fixed sail cone angle is also studied.Through variation of the phase space,the minimum sail lightness number can be obtained by solving a set of algebraic equations instead of a parameter optimization problem.For a given sail lightness number,there are three types of the two-dimensional possible heliocentric motion,including the spiral inward trajectories towards the Sun,the H-reversal trajectories and the directly outward escape trajectories.The boundaries that separate these different groups are easily determined by using the phase space.Finally,the method and procedures to achieve the feasible region of the H-reversal trajectory with required perihelion distance are presented in detail. 展开更多
关键词 solar sail angular momentum reversal (H-reversal) hodograph method
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