低能自由空气电离室优化设计

借助于空气比释动能的基本定义和概念以及空气比释动能绝对测量的理论方法，分析了自由空气电离室可以作为空气比释动能绝对测量方法的原理和条件。通过平板型与圆柱型自由空气电离室的优劣比较，选择平板型作为研究对象，详细介绍了经典的平板型自由空气电离室，并通过理论分析计算以及模拟计算的方法，优化设计包括：光阑半径、空气衰减长度、极间距等低能自由空气电离室的关键几何尺寸，以最小化空气比释动能测量时产生的总不确定度。     

Method of determining the maximum permissible values for diagnostic signs of helicopter transmission units operational status

A method of determining the maximum permissible values for diagnostic signs, being an integral part of health and usage monitoring systems (HUMS) of the helicopter transmission units, has been developed based on a probabilistic approach.     

非线性刚度对微机械陀螺动态性能的影响*

为了提高微机械陀螺的稳定性,研究自由振动状态下活动基座上L-L型双质量微机械陀螺的动态性能,建立微机械陀螺的数学模型,得到以幅值-相位为变量的运动微分方程的解,并给出这种解与轨道元素的联系。研究框架质量和弹性件非线性刚度对陀螺漂移量的影响,并给出数值例子。对所得到的解析关系式与曲线进行分析,作出关于系统性能的相应结论。     

Study of thin-walled parts shaping process based on flanging and embossing

This paper presents the results of analyzing the shaping of thin-walled conical parts with the uniform thickness along generatrix.     

火箭发动机尾部结构优化研究

针对火箭发动机尾部壳体烧穿故障导致系统级失效的突出问题,运用贝叶斯网络模型推得影响系统可靠性的薄弱环节,结合试件性能与残骸分解数据,分析系统故障机理。采用有限元数值计算手段,由流场计算分析固定支架结构破坏后发动机内流场情况,进而明确系统结构优化方案。经结构优化考核试验,火箭发动机外壁温升降低62.17%,系统可靠性提高0.62%,实现可靠性增长的目的。     

OSIRIS-REx: Sample Return from Asteroid (101955) Bennu

In May of 2011, NASA selected the Origins, Spectral Interpretation, Resource Identification, and Security–Regolith Explorer (OSIRIS-REx) asteroid sample return mission as the third mission in the New Frontiers program. The other two New Frontiers missions are New Horizons, which explored Pluto during a flyby in July 2015 and is on its way for a flyby of Kuiper Belt object 2014 MU69 on January 1, 2019, and Juno, an orbiting mission that is studying the origin, evolution, and internal structure of Jupiter. The spacecraft departed for near-Earth asteroid (101955) Bennu aboard an United Launch Alliance Atlas V 411 evolved expendable launch vehicle at 7:05 p.m. EDT on September 8, 2016, on a seven-year journey to return samples from Bennu. The spacecraft is on an outbound-cruise trajectory that will result in a rendezvous with Bennu in November 2018. The science instruments on the spacecraft will survey Bennu to measure its physical, geological, and chemical properties, and the team will use these data to select a site on the surface to collect at least 60 g of asteroid regolith. The team will also analyze the remote-sensing data to perform a detailed study of the sample site for context, assess Bennu’s resource potential, refine estimates of its impact probability with Earth, and provide ground-truth data for the extensive astronomical data set collected on this asteroid. The spacecraft will leave Bennu in 2021 and return the sample to the Utah Test and Training Range (UTTR) on September 24, 2023.

     

Safety Analysis of Helicopter Autorotation Landing Execution on Conditions of Providing Skid Landing Gear Static Strength

The requirements for skid landing gear static strength ensuring are examined based on the comparative analysis of the Airworthiness Standards requirements. Probabilistic principle of determining the safety factor of the skid landing gear is presented. The analysis of the experimental data on bench and flight tests is performed for calculating the actual value of this factor.     

Analytical construction of interception trajectories in atmosphere

For an interception strategy of a removable target by a return space vehicle (RSV), we propose a structure of the control law by the aerodynamic efficiency that determines a chain of the three standard trajectories: nosing-up–free flight–nosing-down. A solution of the terminal problem is to determine numerical values of the control parameters that define moments to switch the RSV flight from one standard trajectory to another.     

The Relativistic Proton Spectrometer (RPS) for the Radiation Belt Storm Probes Mission

The Relativistic Proton Spectrometer (RPS) on the Radiation Belt Storm Probes spacecraft is a particle spectrometer designed to measure the flux, angular distribution, and energy spectrum of protons from ～60 MeV to ～2000 MeV. RPS will investigate decades-old questions about the inner Van Allen belt proton environment: a nearby region of space that is relatively unexplored because of the hazards of spacecraft operation there and the difficulties in obtaining accurate proton measurements in an intense penetrating background. RPS is designed to provide the accuracy needed to answer questions about the sources and losses of the inner belt protons and to obtain the measurements required for the next-generation models of trapped protons in the magnetosphere. In addition to detailed information for individual protons, RPS features count rates at a 1-second timescale, internal radiation dosimetry, and information about electrostatic discharge events on the RBSP spacecraft that together will provide new information about space environmental hazards in the Earth’s magnetosphere.