Deep Impact: Working Properties for the Target Nucleus – Comet 9P/Tempel 1

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide observing campaign (Meech et al., Space Sci. Rev., 2005a). This campaign has already produced a great deal of information on the global properties of the comet’s nucleus (summarized in Table I) that is vital to the planning and the assessment of the chances of success at the impact and encounter. Since the mission was begun the successful encounters of the Deep Space 1 spacecraft at Comet 19P/Borrelly and the Stardust spacecraft at Comet 81P/Wild 2 have occurred yielding new information on the state of the nuclei of these two comets. This information, together with earlier results on the nucleus of comet 1P/Halley from the European Space Agency’s Giotto, the Soviet Vega mission, and various ground-based observational and theoretical studies, is used as a basis for conjectures on the morphological, geological, mechanical, and compositional properties of the surface and subsurface that Deep Impact may find at 9P/Tempel 1. We adopt the following working values (circa December 2004) for the nucleus parameters of prime importance to Deep Impact as follows: mean effective radius = 3.25± 0.2 km, shape – irregular triaxial ellipsoid with a/b = 3.2± 0.4 and overall dimensions of ∼14.4 × 4.4 × 4.4 km, principal axis rotation with period = 41.85± 0.1 hr, pole directions (RA, Dec, J2000) = 46± 10, 73± 10 deg (Pole 1) or 287± 14, 16.5± 10 deg (Pole 2) (the two poles are photometrically, but not geometrically, equivalent), Kron-Cousins (V-R) color = 0.56± 0.02, V-band geometric albedo = 0.04± 0.01, R-band geometric albedo = 0.05± 0.01, R-band H(1,1,0) = 14.441± 0.067, and mass ∼7×10¹³ kg assuming a bulk density of 500 kg m⁻³. As these are working values, {i.e.}, based on preliminary analyses, it is expected that adjustments to their values may be made before encounter as improved estimates become available through further analysis of the large database being made available by the Deep Impact observing campaign. Given the parameters listed above the impact will occur in an environment where the local gravity is estimated at 0.027–0.04 cm s⁻² and the escape velocity between 1.4 and 2 m s⁻¹. For both of the rotation poles found here, the Deep Impact spacecraft on approach to encounter will find the rotation axis close to the plane of the sky (aspect angles 82.2 and 69.7 deg. for pole 1 and 2, respectively). However, until the rotation period estimate is substantially improved, it will remain uncertain whether the impactor will collide with the broadside or the ends of the nucleus.     

上证指数"百点效应"实证研究——基于前景理论的分析

通过研究上证指数落在百点附近区间的频率和日K线图的表现，揭示了其分布规律和运行特征。实证结果表明，从市场总体看，百点区间内样本较大时上证指数落在百点附近区间的频率接近均匀分布时的概率，上涨行情时，越过大多数百点位比较困难，而下跌行情时比较容易，百点位在某段行情的稳定性与上证指数在该百点附近区间的横盘整理时间有关。     

离散事件系统的Petri网图仿真

1.前言 离散事件动态系统DEDS(Discrete Event Dynamic System)的传统分析方法——应用排队论和随机过程理论为离散事件动态系统建立排队网络模型,在很多情况下已不适用。新的理论和研究方法相继提出。其中之一是“皮特里网”(Petri Nets)理论。另一种比较成熟的方法是仿真法,但是,仿真法要以高昂的计算机设备的大量计算时间为代     

航天飞机三维最优再入轨道及气动加热过程

本文应用现代控制理论研究了航天飞行器三维最优再入轨道和与轨道参数密切相关的气动加热过程。文中选择飞行器迎角和倾斜角作为控制变量,以飞行器气动加热率和飞行过载沿轨道积分最小作为优化性能指标,按极大原理导出最优再入轨道有约束控制的非线性两点边值问题。采用了数值优化方法——共轭梯度法求解有升力飞行器的最优再入轨道及其热过程。文中以允许误差法讨论了权系数和罚函数的选取方法;对不同速度范围研究了不同的加热模型;按热平衡方程与优化轨道同步迭代的方法求得了算例数值结果。算例的数值结果与文献[13]的量值是一致的。     

三维可压缩混合层中扰动演化的研究

为了利用被动控制增强可压缩混合层中混合效率,本文用数值模拟的方法研究了三维可压缩混合层中扰动向下游的演化.通过在入口处引入不同的不稳定T-S波,给出了扰动随空间的演化过程,及马赫数对扰动演化的影响.计算结果表明在马赫数较小时,扰动波增长很快,当马赫数增大时,扰动所形成的流向涡的强度会减弱.这一结论与流动稳定性分析结果是一致的.     

无穷观问题的研究(Ⅲ)——‘每一''与‘所有''

本组系列论文（I）－（Ⅴ）从数学和认识论的角度系统地研究了无穷观问题的历史发展和现状，确立了无穷观背景世界的三分法原则，指出了两种穷观相互排斥的局限性，形成了统一两种无穷于同一框架中的基本观点，并建立了一个统一实无限与潜无限于同一框架中的公理集合论系统APAS。     

中介时序逻辑系统MTL的模型论性质

时序逻辑作为一种把时间概念直接引入其形式系统的逻辑系统,它具有较强的表达能力,近年来在计算机科学领域获得了广泛的应用.基于中介逻辑对时序逻辑进行多值扩充,建立了一种中介时序逻辑系统MTL(Medium Temporal Logic).讨论了它的形式系统和语义解释,但未论及其完备性.本文对MTL系统作进一步的讨论.在一可传结构下,讨论了它的可传、连通和过滤等模型论性质,为进一步讨论MTL系统的完备性作了理论上的准备.     

空天飞机的边界层转捩

本文概述了边界层转捩对空天飞机性能的影响。在介绍确定边界层转捩起始点的线性稳定性理论和简单关联公式之后，又从噪声影响、头部钝头影响和钝锥飞行试验结果等几方面，讨论了线性稳定性理论的应用。接着介绍了采用转捩函数来确定转捩区的方法。从飞行试验、理论计算和风洞试验等三方面，探讨了进一步研究高超声速边界层转捩的途径。重点介绍了ＮＡＳＡＬａｎｇｌｅｙ研究中心的超声速、高超声速静风洞技术的发展。最后，对今后空天飞机边界层转捩的研究工作提出了建议。     

航天飞行中的稀薄气体动力学

飞船、宇航探测器、航天飞机等复杂外形航天器给气体动力学，包括稀薄气体动力学提出了新的要求。本文简要介绍了为计算过渡领域中气动力与热而发展的基于位置元概念的DSMC方法的通用算法。该方法解决了计算物面通量量的技术难点并已用于模拟圆球、飞船、类航天飞机的绕流。正在进行的航天实践，如麦哲伦飞船对金星的探测、行星大气中的气动制动、伽利略飞船的木星之行、尾屏蔽在太空中获得高真空的实验等等提出了新的气动力问题，稀薄气体动力学和DSMC方法是有力的工具。