Oblique detonation wave triggered by a double wedge in hypersonic flow

Pressure-gain combustion has gained attention for airbreathing ramjet engine applications owing to its better thermodynamic efficiency and fuel consumption rate. In contrast with traditional detonation induced by a single wedge, the present study considers oblique shock interactions attached to double wedges in a hypersonic combustible flow. The temperature/pressure increases sharply across the interaction zone that initiates an exothermic reaction, finally resulting in an Oblique Detonation Wav...     

空气分配对双旋流燃烧室性能影响的试验研究

为了研究燃气轮机燃烧室主燃区和掺混区空气分配比例对燃烧室性能的影响,在双旋流环形燃烧室上进行全温全压燃烧试验研究。结果表明,随运行工况的提高,燃烧室出口温度分布系数OTDF呈现总体降低的变化趋势,出口径向温度分布系数RTDF呈现先显著降低、后缓慢升高并最终平稳的变化趋势,总压恢复系数略有增加;随着主燃区空气比例的增加,OTDF呈现先增加再降低再增加的变化趋势,并在主燃区空气比例为0.343时达到最小值;随掺混区空气比例的增加,燃烧室RTDF持续降低;主燃区和掺混区的进气比例对燃烧室的总压恢复系数几乎没有影响。     

双S弯喷管的流固耦合特性研究

为了明晰S弯喷管的流固耦合特性,数值模拟了流固耦合作用下双S弯收敛喷管的结构变形特征及其内/外流特性。结果表明：S弯喷管的圆转方弯曲构型产生了非均匀的流场分布,并增强了结构的弹性特征,它们通过交换气动载荷与变形位移数据形成了S弯喷管流固耦合的作用机理。在气动载荷作用下,S弯喷管沿Y向的最大变形位移为25.3mm,它位于喷管出口上壁面的中心位置。当喷管的结构变形稳定时,第二弯转弯处下壁面的气流加速至局部超音速,壁面静压大幅降低;第一弯下游上壁面附近形成了气流分离区;喷管出口喷流沿轴向向上偏转。流固耦合作用导致S弯喷管的流量系数减小0.6%,推力系数降低1.8%。矩形截面与弯曲构型是影响S弯喷管流固耦合特性的主要几何特征,其中矩形截面能够显著增大喷管的变形位移;S形弯曲构型虽然能够有效抑制变形特征,但它导致喷管多个区域出现变形,喷管的结构变形分布变得更加复杂。     

The James Webb Space Telescope (JWST)

The James Webb Space Telescope is a 6.5 m, infrared space telescope designed to be launched in 2013 aboard an Ariane 5. The JWST program is a cooperative program with the Goddard Space Flight Center (GSFC) managing the project for NASA. The prime contractor for JWST is Northrop Grumman Space Technology (NGST). JWST’s international partners are the European Space Agency (ESA) and the Canadian Space Agency (CSA). JWST will address four major science themes: end of the dark ages: first light and reionization; the assembly of galaxies, the birth of stars and protoplanetary systems; and the formation of planetary systems and the origins of life. We discuss the design of the observatory and review recent progress on the JWST program.     

恒星地球模拟器的光学系统设计与精度模拟分析研究

为实现对敏感器的地面标定与精度测试, 需研制一套恒星地球模拟器, 要求其星间角距模拟精度优于10", 地球张角模拟精度优于0.05°. 通过设计高精度准直光学系统与高精度紫外准直光学系统, 实现了对星点位置与地球图像的无穷远距离模拟; 提出了星点位置模拟误差修正方法与地球图形模拟误差修正方法, 提高星间角距和地球张角的模拟精度.实测星间角距与地球张角模拟结果表明, 该模拟器的星间角距模拟精度优于10", 地球张角模拟精度优于0.02°.     

光谱连续可调星敏感器地面标定系统设计

为解决由于色温不匹配对星敏感器光信号定标精度产生的影响,提出一种光谱连续可调星敏感器地面标定系统设计方案.该高精度准直光学系统的光谱范围为500~800nm,像质测试结果表明,全视场畸变小于0.08%,MTF在60lp·mm^-1处大于0.6.基于DMD光源系统的组成和工作原理,对光谱分辨率和光谱曲线模拟精度进行分析,设计了一套光谱分辨率全谱段优于2nm的Czerny-Turner分光系统.测试结果表明,星点位置精度优于7";光谱分辨率为10nm和20nm时光谱曲线模拟精度分别优于2%和5%,有效降低了由于色温不匹配对星敏感器标定精度的影响.

     

Improvement of the GRACE star camera data based on the revision of the combination method

The new release of the sensor and instrument data (Level-1B release 02) of the Gravity Recovery and Climate Experiment (GRACE) had a substantial impact on the improvement of the overall accuracy of the gravity field models. This has implied that improvements on the sensor data level can still significantly contribute to arriving closer to the GRACE baseline accuracy. The recent analysis of the GRACE star camera data (SCA1B RL02) revealed their unexpectedly higher noise. As the star camera (SCA) data are essential for the processing of the K-band ranging data and the accelerometer data, thorough investigation of the data set was needed. We fully reexamined the SCA data processing from Level-1A to Level-1B with focus on the combination method of the data delivered by the two SCA heads. In the first step, we produced and compared our own combined attitude solution by applying two different combination methods on the SCA Level-1A data. The first method introduces the information about the anisotropic accuracy of the star camera measurement in terms of a weighing matrix. This method was applied in the official processing as well. The alternative method merges only the well determined SCA boresight directions. This method was implemented on the GRACE SCA data for the first time. Both methods were expected to provide optimal solution characteristic by the full accuracy about all three axes, which was confirmed. In the second step, we analyzed the differences between the official SCA1B RL02 data generated by the Jet Propulsion Laboratory (JPL) and our solution. SCA1B RL02 contains systematically higher noise of about a factor 3–4. The data analysis revealed that the reason is the incorrect implementation of algorithms in the JPL processing routines. After correct implementation of the combination method, significant improvement within the whole spectrum was achieved. Based on these results, the official reprocessing of the SCA data is suggested, as the SCA attitude data are one of the key observations needed for the gravity field recovery.     

Precision analysis of autonomous orbit determination using star sensor for Beidou MEO satellite

This paper focuses on the autonomous orbit determination accuracy of Beidou MEO satellite using the onboard observations of the star sensors and infrared horizon sensor. A polynomial fitting method is proposed to calibrate the periodic error in the observation of the infrared horizon sensor, which will greatly influence the accuracy of autonomous orbit determination. Test results show that the periodic error can be eliminated using the polynomial fitting method. The User Range Error (URE) of Beidou MEO satellite is less than 2?km using the observations of the star sensors and infrared horizon sensor for autonomous orbit determination. The error of the Right Ascension of Ascending Node (RAAN) is less than 60?$\mathrm{\mu }\text{rad}$ and the observations of star sensors can be used as a spatial basis for Beidou MEO navigation constellation.     

Shocklike soliton because of an impinge of protons and electrons solar particles with Venus ionosphere

This paper introduces an investigation of shocklike soliton or small amplitude Double Layers (DLs) in a collisionless plasma, consisting of positive and negative ions, nonthermal electrons, as well as solar wind streaming protons and electrons. Gardner equation is derived and its shocklike soliton solution is obtained. The model is employed to recognize a possible nonlinear wave at Venus ionosphere. The results indicate that the number densities and velocities of the streaming particles play crucial role to determine the polarity and characteristic features (amplitude and width) of the shocklike soliton waves. An electron streaming speed modifies a negative shocklike wave profile, while an ion streaming speed modulates a positive shocklike wave characteristic.     

螺旋管成形模具的CAD/CAM方法研究

针对螺旋管成形模具的特点,采用Pro/Engineer进行三维实体设计、PowerMILL进行数控编程的设计制造方法,充分发挥Pro/Engineer三维实体的参数化设计和PowerMILL刀具路径轨迹优化的优势,缩短了螺旋管成形模具的设计制造周期,提高了螺旋管成形模具的加工精度。