Small-Scale Solar Magnetic Fields

As we resolve ever smaller structures in the solar atmosphere, it has become clear that magnetism is an important component of those small structures. Small-scale magnetism holds the key to many poorly understood facets of solar magnetism on all scales, such as the existence of a local dynamo, chromospheric heating, and flux emergence, to name a few. Here, we review our knowledge of small-scale photospheric fields, with particular emphasis on quiet-sun field, and discuss the implications of several results obtained recently using new instruments, as well as future prospects in this field of research.     

Testing the Stability of the Fine Structure Constant in the Laboratory

In this review we discuss the progress of the past decade in testing for a possible temporal variation of the fine structure constant α. Advances in atomic sample preparation, laser spectroscopy and optical frequency measurements led to rapid reduction of measurement uncertainties. Eventually laboratory tests became the most sensitive tool to detect a possible variation of α at the present epoch. We explain the methods and technologies that helped to make this possible.     

Integrated Planning and Execution for Autonomous Spacecraft

An autonomous spacecraft must balance long-term and short-term considerations. It must perform purposeful activities that ensure long-term science and engineering goals are achieved and ensure that it maintains positive resource margins. This requires planning in advance to avoid a series of shortsighted decisions that can lead to failure. However, it must also respond in a timely fashion to a somewhat dynamic and unpredictable environment. Thus, in terms of high-level, goal-oriented activity, spacecraft plans must often be modified due to fortuitous events such as early completion of observations and setbacks such as failure to acquire a guidestar for a science observation. This describes an integrated planning and execution architecture that supports continuous modification and updating of a current working plan in light of a changing operating context.     

用于波音787的新型复合材料机翼除冰系统

在机械系统方面,现代商业飞机通常采用一系列管道从发动机内部引入加热的空气,通过加热空气在结冰机翼表面内侧的流动加热附近的机翼表面,从而达到除冰的目的。但是这不仅会使设计变得复杂,同时还会降低发动机的有效推力。所以,多年来研究人员一直在开发一种替代技术,即向机翼前缘表层里面置入导电元件来直接加热机翼表面,使冰层不会聚集变厚。     

UG NX在数控编程中的应用技巧

随着CAD、CAM、CAE等技术的不断发展和日趋完善,它们在各个领域得到了极其广泛的应用.     

开放进化式切削数据平台的开发应用

自1964年10月美国金切联合研究公司建立了第1个金属切削数据库以来,世界各国相继建立了各种切削数据库.计算机技术的飞速发展促使人们对切削参数的选取提出了更高的要求,切削参数的数字化和共享化已经成为大势所趋.     

多控制面机翼阵风减缓主动控制与风洞试验验证

针对某大展弦比多控制面弹性机翼风洞模型,分别从频域和时域进行阵风响应分析和阵风响应减缓控制律设计.采用经典控制理论设计控制律,通过操纵位于0.6和0.8翼展处的内外侧控制面减小由正弦阵风引起的翼尖加速度(WTA).低频段的阵风减缓的数值分析与风洞试验结果均表明:多控制面的阵风减缓效果优于单控制面.当来流速度为14 m/s时,针对频率为2～5 Hz的阵风,采用多控制面得到的WTA减小10%～24%;当来流速度在8～16 m/s时,针对频率为2 Hz的正弦阵风,闭环状态下的翼尖加速度减小10%～40%;结构有限元模型与真实模型存在工程允许的误差导致理论与试验结果存在一定的误差.本文的工作对工程实际中采用阵风减缓技术具有参考价值.     

Investigation of the infrared characteristics of the rocket nozzle

Investigation of the infrared characteristics of a rocket nozzle is very important for the study of infrared initiating technology. The Narrow-Band Zone model is developed for that purpose. The spectral transmission and absorption factors are introduced, and the equations between radiative heat flux and the temperature of waill surfaces and gas are developed. The radiative heat transfer in one axisymmetric cylindrical enclosure filled with homogeneous radiative participating medium is computed with the Narrow-Band Zone model and compared with those in the reference documents. The comparison shows good agreement. The radiative heat transfer to the nozzle of one rocket engine is also calculated with the Narrow-Band Zone model, and the outgoing radiative energy flux and energy rate integrated in a mid-wave infrared band 2-6 pm, a long-wave infrared band 8-14 pm and the full wave band are analyzed. The following conclusions can be derived: the spectral radiation from the inlet and outlet of the nozzle show apparent spectral discontinuity, which appears greater in the 2.7-2.95 pm than in the neighboring wave band. The spectral outgoing radiative energy flux of nozzle wail is similar to that of gray body, which decreases with wavelength in 2-14 pm. The outgoing radiative energy flux on the nozzle wall is greater in the cylindrical and contracting section of nozzle, but smaller in the divergent section, which is determined by temperature. The nozzle of the rocket engine radiates most energy in the mid-wave surfaces by absorption. The most important feature of gas radiation is the strong selection of the waveband, so the detailed study of the infrared characteristics of nozzle of the rocket engine should be carried out on narrow-band computation.     

模态综合的直接变换法

基于固定界面模态综合的Craig-Bampton方法,提出了模态综合的直接变换方法,该法在形式上更简洁,适用于大规模动力学系统的模态分析和动力学模型减缩。对采用直接变换法模态综合过程的计算误差做了分析,给出了计算误差界,阐明了模态综合后总体结构的固有频率与子结构保留主模态个数之间的关系。针对子结构界面自由度太大的情况,提出了直接变换法的分部算法,不需组集系统总刚度、总质量矩阵,仅在子结构的基础上完成系统的减缩。计算实例表明该算法的有效性及计算的稳定性。