飞机稳定尾旋的预测研究

在考虑各种影响因素的基础上，增加了交叉惯性积对稳定尾旋的影响，从而导出了分析稳定尾旋的有关公式。为了避免遗漏解的可能性，采用不需选择初值的求解方法，给出了稳定尾旋的判据。应用该方法对某型飞机的尾旋进行了预测计算，求出了一个陡尾旋解和一个平尾旋解，计算结果与该飞机尾旋试飞结果吻合较好，表明计算方法是正确的，计算结果可用于指导飞机的尾旋试飞。     

论中小企业信用评价及其融资

本文通过对中小企业信用评价的分析研究，以破解其融资难问题，有利于促进中小企业健康的发展。     

一种新型二元风洞侧壁干扰修正方法——当地修正法

针对现行总体型二元风洞侧壁干扰修正方法的不合理性，本文发展了一种新型修正方法——当地修正法，并就有关问题做了讨论。与目前的总体型方法相比，当地修正法致力于对模型当地流动参数的修正，而不是笼统地去调整试验条件。当地修正法有能力处理那些主要的侧壁边界层效应及相关问题，是未来开展侧壁干扰修正的一条有效途径。     

New evidence for strong non-thermal effects in Tycho’s supernova remnant

For the case of Tycho’s supernova remnant (SNR), we present the relation between the blast wave and contact discontinuity radii calculated within the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is demonstrated that these radii are confirmed by recently published Chandra measurements which show that the observed contact discontinuity radius is very close to the shock radius. Therefore a consistent explanation of these observations can be given in terms of efficient CR acceleration which makes the medium more compressible.     

无穷多项和求极限问题的探讨

针对求极限过程中的一个难点———无穷多项和求极限 ,可通过先求和、夹逼定理、无穷小分析法、定积分等四种方法加以解决。     

高职教育与生产实践相结合刍论

目前,我国高等职业教育蓬勃发展,但仍存在着教育与实践结合不够紧密的问题,要解决这一问题,首先要加强教材建设,编制出实用性的教材。其次专业课教师必须是"双师型",同时要学习发达国家高职教育的先进理念,早日实现教育与生产实践的结合。     

Crew autonomy for deep space exploration: Lessons from the Antarctic Search for Meteorites

Future piloted missions to explore asteroids, Mars, and other targets beyond the Moon will experience strict limitations on communication between vehicles in space and control centers on Earth. These limitations will require crews to operate with greater autonomy than any past space mission has demonstrated. The Antarctic Search for Meteorites (ANSMET) project, which regularly sends small teams of researchers to remote parts of the southern continent, resembles a space mission in many ways but does not rely upon a control center. It provides a useful crew autonomy model for planners of future deep space exploration missions. In contrast to current space missions, ANSMET gives the crew the authority to adjust competing work priorities, task assignments, and daily schedules; allows the crew to be the primary monitor of mission progress; demands greater crew accountability for operational errors; requires the crew to make the most of limited communication bandwidth; adopts systems designed for simple operation and failure recovery; and grants the crew a leading role in the selection and stowage of their equipment.     

民用航空器优先权研究

在民用航空器权利中，民用航空器优先权是一种重要的权利，然而该荐权利仅仅规定在特别法中，在中国还没有设立统一的优先权制度。随着中国物权法的立法步伐的加快，深入研究优先权这一传统担保物权已成为不容回避的问题。为此，拟通过对民用航空器优先权的研究，推动物权方法，指导司法实践。     

《机械制造技术》课程特点与现场教学

《机械制造技术》课程具有很强的综合性和实践性、教学难度大的特点。教学中要以理论教学和现场教学相结合的方法，以提高教学效率和质量。同时要正确选择课题、设计合适的教学方法是改革现场教学的主要措施。     

The evolution of mirror type magnetic fluctuations in the magnetosheath based on multipoint observations

Two orbits were selected in January–February 2006 when the separation between the Cluster spacecraft was large and mirror type magnetic field fluctuations were observed by all spacecraft in different regions of the terrestrial magnetosheath. Minimum variance analysis was applied to find the mirror type fluctuations, and the amplitude of the fluctuations was determined individually. Mirror mode structures are moving along the streamlines frozen in the plasma. A model was developed for the calculation of plasma flowtime from the bow shock to the observation point. The growth rate of the field strength perturbations was estimated by comparing the amplitudes of fluctuations observed simultaneously at distant locations (∼10,000 km) based on the assumption that δB ∼ exp(γt). The obtained growth rate values were about an order of magnitude smaller than those provided by linear models and they decreased in the inner regions of the magnetosheath, indicating some saturation in the growth of the waves when proceeding towards the magnetopause. The results of these two case studies suggest that mirror type fluctuations originate from the compression region downstream of the quasi-perpendicular bow shock, and the growth of the fluctuations cannot be described by linear approximations.