宽带双极化天线测量探头的设计与仿真

天线测量探头的性能对提升天线平面近场测量效率、最终测量结果的精度具有重要意义。针对平面近场测量的需要，应用反向四脊和差分馈电技术，设计了宽带双极化天线测量探头。对测量探头模型进行仿真，分析了带宽、方向图、隔离度和交叉极化辨识度等探头性能，确定了高隔离度、高极化纯度的宽带双极化天线测量探头的最优设计，获得了更高精度和效率的天线测量。     

弯刀装置的倾斜和横向位移测量

阐述了对４ｍ×３ｍ风洞弯刀装置的倾斜和横向位移测量的项目内容，详细介绍了测量方案和具体的测量方法，分析了测量结果，并说明了该项测量任务的应用价值和实际意义。     

基于里德堡原子相干效应的微波电场测量技术研究进展

近年来，采用里德堡原子的微波电场测量技术得到了迅速发展，获得了广泛应用。该电场探测技术是一项全新技术，可以将微波电场通过基本物理常数与频率测量直接关联，具有测量动态范围大、测量灵敏度高和测量不确定度小的特点，有望替代传统溯源路径，直接关联国际单位制（SI）。本文基于里德堡原子相干效应的微波电场测量技术原理，针对国内外微波电场的高准确度、高灵敏度和极化方向测量技术发展现状，和对微波电场测量的工程化光源系统，蒸气室探头的仿真验证实验和集成式蒸气室探头的设计研究等方面的相关进展做了详细介绍。     

超量程位置误差基准桥接测量技术研究

以某类型专用检具为例，介绍了一种基于坐标测量机的利用基准桥接测量其位置误差的方法，对平行度和垂直度参数建立了数学模型并进行了计算推导，给出了实现测量的方法，提升了测量范围和测量能力，同时对测量结果不确定度进行了评定，证实了此方法的可行性。     

带校准源的电压测量系统

研究了由分压器和模数转换器组成的电压测量系统在有校准源的情况下，为提高测量准确度，如何实施测量和数据处理的问题，并给出了实验结果     

超精密球度的激光干涉测量方法

传统的球度测量方法很难达到亚微米级的测量准确度。为此，提出了超精密球度激光干涉测量的新方法，介绍了测量装置的结构及测量原理，并给出了球面波和球度计算的数学模型。     

一种基于斜向观测的镜面法线方向测量方法

针对航天器上平面镜、立方镜等镜面法线方向测量时，准直光路被遮挡的情况，提出了一种斜向观测方法，即通过两台经纬仪在镜面法线两侧对称位置互相观测平行光的方法，获得镜面法线方向。对测量对象进行了说 明，详细描述了镜面法线准直测量原理和斜向观测原理，根据两种测量方法开展了测量比对试验，给出了过程观测 数据和计算结果。通过多次试验数据统计，斜向观测结果与准直测量结果差异在角秒量级，满足航天器测试要求，可以有效解决在航天器上基准镜面准直方向被遮挡时法线方向测量的难题。     

光电自准直经纬仪水平角测量误差分析

针对光电自准直经纬仪的水平角测量原理和系统组成特点，全面分析了影响其水平角测量精度的各项误差分量，并对各种误差因素进行了定量计算，对系统误差提出补偿方法。通过分析和补偿，可将光电准直经纬仪水平角测量精度提高到0.5″，满足Ⅰ等电子经纬仪的测量精度指标。     

光栅式传动链误差测量系统的不确定度分析

为了进一步改善传动链误差测量系统的性能，以谐波减速器为被测对象，通过推导测量系统不确定度评定的一般方法，找出了测量系统的各个不确定度分量；通过分析系统中A类和B类不确定度，阐述了各个不确定度分量对整个测试系统的影响，提出了减少不确定度的相关措施，为优化传动误差测量系统的测量提供了指导。     

提高GPS实时测量准确度的方法

介绍了ＧＰＳ实时测量应用的背景，并论述了两种提高ＧＰＳ测量准确度的方法：差分ＧＰＳ法和载波相位法，并给出了作者应用ＤＧＰＳ测量的数据。     

Exploration of groundwater potential zones mapping for hard rock region in the Jakham river basin using geospatial techniques and aquifer parameters

Geospatial techniques are useful to understand the groundwater resources assessment, development, and management. Groundwater mapping is essential to counter the excessive withdrawal of groundwater and fulfil the need of drinking, irrigation water in hard rock areas. Currently, the main problem is facing the groundwater level is decreasing due to less rainfall, climate changes and increasing demand, which is under in the hot zones. This results can be more useful for future challenges, sustainable development and demand to Jakham river basin. The main objective of this paper to demarcated the groundwater potential zones (GWPZ) using geospatial techniques for the hard rock region with the reference of aquifer parameters. In this paper, we have used to total eight thematic layers such as geomorphology, land use, soil, topographic elevation, slope, post-monsoon groundwater level (GWL), net recharge, and transmissivity, which are prepared from satellite data and field verification. All thematic layers were integrated for assigning the weights to demarcation of the groundwater potential zones in the RS and GIS environment. The selected thematic layers and features were assigned weightage and normalized by the analytic hierarchy process (AHP) technique. Finally, the thematic layers were systematically integrated using weighted overlay analysis within a GIS environment. We have classified into five GWPZ classes i.e. very high, high, moderate, low, and very low for basin area using GIS, and AHP methods. The study area result indicated that high and moderate zone, which is confined in the central part of the basin, covers 2.43 % and 43.88 % area, respectively. The low (49.21 %) and very low (4.25%) GW potential zone is under the confined aquifer in the high slope and rock outcrops formations near the basin boundary. The final GWPZ map was validated with groundwater level fluctuation data, which illustrates the accuracy of the adopted approach. This unique approach and conclusions of this work may also help to develop the framework and policies for swiftly analyzing groundwater recharge planning, development and locating the artificial recharge structures in the other semi-arid, arid and hard rock regions.     

An extension of HZETRN for cosmic ray initiated electromagnetic cascades

Safe and efficient mission operations in space require an accurate understanding of the physical interactions of space radiation. As the primary space radiation interacts with intervening materials, the composition and spectrum of the radiation environment changes. The production of secondary particles can make a significant contribution to radiation exposure. In this work, the NASA space radiation transport code, HZETRN, is extended to include the transport of electrons, positrons, and photons. The production of these particles is coupled to the initial cosmic ray radiation environment through the decay of neutral pions, which produce high energy photons, and through the decay of muons, which produce electrons and positrons. The photons, electrons, and positrons interact with materials producing more photons, electrons and positrons generating an electromagnetic cascade. The relevant cross sections, transport equation, and solution method are introduced. Electron and positron production in Earth’s atmosphere is investigated and compared to experimental balloon-flight measurements. Reasonable agreement is seen between HZETRN and data.     

New results and questions of lunar exploration from SELENE,Chang’E-1, Chandrayaan-1 and LRO/LCROSS

The moon has longstanding questions such as lunar environments, origin, formation and evolution, magnetization of crustal rocks, internal structure and possible life. The recent lunar missions, e.g., SELenological and ENgineering Explorer “KAGUYA” (SELENE), Chang’E-1, Chandrayaan-1, and Lunar Reconnaissance Orbiter/Lunar CRater Observation and Sensing Satellite (LRO/LCROSS), have provided new opportunities to explore and understand these issues. In this paper, we reviewed and presented the results and findings in the fields of lunar gravity, magnetic field, atmosphere, surface geomorphology and compositional variations, volcano, craters, internal structure, water and life science from new lunar exploration missions. In addition, the new objectives and scientific questions on lunar explorations in near future are presented and discussed.     

Integration of In-Situ Resource Utilization into lunar/Mars exploration through field analogs

The ability to extract and process resources at the site of exploration into useful products such as propellants, life support and power system consumables, and radiation and rocket exhaust plume debris shielding, known as In-Situ Resource Utilization or ISRU, has the potential to significantly reduce the launch mass, risk, and cost of robotic and human exploration of space. The incorporation of ISRU into missions can also significantly influence technology selection and system development in other areas such as power, life support, and propulsion. For example, the ability to extract or produce large amounts of oxygen and/or water in-situ could minimize the need to completely close life support air and water processing system cycles, change thermal and radiation protection of habitats, and influence propellant selection for ascent vehicles and surface propulsive hoppers. While concepts and even laboratory work on evaluating and developing ISRU techniques such as oxygen extraction from lunar regolith have been going on since before the Apollo 11 Moon landing, no ISRU system has ever flown in space, and only recently have ISRU technologies been developed at a scale and at a system level that is relevant to actual robotic and human mission applications. Because ISRU hardware and systems have never been demonstrated or utilized before on robotic or human missions, architecture and mission planners and surface system hardware developers are hesitant to rely on ISRU products and services that are critical to mission and system implementation success. To build confidence in ISRU systems for future missions and assess how ISRU systems can best influence and integrate with other surface system elements, NASA, with international partners, are performing analog field tests to understand how to take advantage of ISRU capabilities and benefits with the minimum of risk associated with introducing this game-changing approach to exploration. This paper will describe and review the results of four analog field tests (Moses Lake in 6/08, Mauna Kea in 11/08, Flagstaff in 9/09, and Mauna Kea in 1/10) that have begun the process of integrating ISRU into robotic and human exploration systems and missions, and propose future ISRU-related analog field test activities that can be performed in collaboration with non-US space agencies.     

Quality characteristics of the radish grown under reduced atmospheric pressure

This study addresses whether reduced atmospheric pressure (hypobaria) affects the quality traits of radish grown under such environments. Radish (Raphanus sativus L. cv. Cherry Bomb Hybrid II) plants were grown hydroponically in specially designed hypobaric plant growth chambers at three atmospheric pressures; 33, 66, and 96 kPa (control). Oxygen and carbon dioxide partial pressures were maintained constant at 21 and 0.12 kPa, respectively. Plants were harvested at 21 days after planting, with aerial shoots and swollen hypocotyls (edible portion of the radish referred to as the “root” hereafter) separated immediately upon removal from the chambers. Samples were subsequently evaluated for their sensory characteristics (color, taste, overall appearance, and texture), taste-determining factors (glucosinolate and soluble carbohydrate content and myrosinase activity), proximate nutrients (protein, dietary fiber, and carbohydrate) and potential health benefit attributes (antioxidant capacity). In roots of control plants, concentrations of glucosinolate, total soluble sugar, and nitrate, as well as myrosinase activity and total antioxidant capacity (measured as ORAC_FL), were 2.9, 20, 5.1, 9.4, and 1.9 times greater than the amount in leaves, respectively. There was no significant difference in total antioxidant capacity, sensory characteristics, carbohydrate composition, or proximate nutrient content among the three pressure treatments. However, glucosinolate content in the root and nitrate concentration in the leaf declined as the atmospheric pressure decreased, suggesting perturbation to some nitrogen-related metabolism.     

GNSS-Reflectometry: Forest canopies polarization scattering properties and modeling

Nowadays, GNSS-Reflectometry (GNSS-R) can be a new promising remote sensing tool in the ocean, snow/ice and land surfaces, e.g., vegetation biomass monitoring. Although GNSS-R provides a potentially special L-band multi-angular and multi-polarization measurement, the theoretical vegetation scattering properties and mechanisms for GNSS-R are not understood clearly. In this paper, the GNSS-R vegetation polarization scattering properties are studied and modeled at different incidence angles (specular direction). The bistatic scattering model Bi-mimics is employed, which is the first-order radiative transfer equation. As a kind of forest stand, the Aspen’s crown layer is composed of entire leaves, and its parameters in Mimics handbook are used as model input. The specular circular polarizations (co-polarization RR and cross-polarization LR) are simulated. For cross-polarization, the received polarization is assumed as a linear (horizontal and vertical) polarizations and ±45° linear polarizations. Therefore, the HR VR, +45R and −45R polarizations are simulated here. Contributions from different scattering components at RR, LR and VR polarization are also presented. For co-polarization, it is large in the whole specular angles (10–80°). The scattering trends of the other cross polarization (HR, LR, +45R and −45R) are a little similar when compared to the RR and RV. Therefore, the RHCP and V polarizations are more favorable to collect the reflected signals. The trunk heights and crown depths do not affect the scattering trends of RR, RV and RL, while the trunk height has some effect on the scattering amplitude of different polarizations. The azimuth angle has more effects on RR, RL and RV scattering, especially in lower than 50°. The observation angles and polarization combinations are extremely important for GNSS-R remote sensing.     

流星参数的数值分析和流星高度分布模型

流星余迹能够被后向散射雷达观测到, 利用观测结果, 可以分析和研究流星的空间分布和时间变化规律. 同时, 利用流星空间分布还可以进行空间碎片的研究. 基于标准理论, 对影响雷达回波功率的主要因素, 例如如双极扩散、余迹的初始半径、流星的有限速度, 以及雷达的脉冲重复频率在不同频率和速度下进行了数值分析和计算, 得到的流星衰减时间及双极扩散系数的观测结果与理论结果一致. 通过对昆明流星雷 达观测到的571632个流星进行统计分析, 得到了流星高度分布统计模型, 并利用该模型的分析结果与不同月份流星的观测数据进行对比, 结果比较一致.      

绳驱动机器人的解耦分析和位置控制仿真

为提高机器人的负载能力,基于几何分析和螺旋理论的基本原理,对绳驱动 拟人臂机器人的构型设计、钢绳传动方式和运动学控制问题进行了深入的分析.首先针对绳 驱动走线方式的多样性选择,设计了一种具有肘、腕关节耦合和肩、肘关节耦合的绳驱动传 动机构;然后以肩、肘、腕7-DOF关节为中间媒介对机器人末端和驱动钢绳间的运动学关系 进行了分析,即先考虑机器人末端位姿和各关节角度之间的关系,再研究各关节角度和其相 应的驱动钢绳绳长之间的关系,从而得到绳驱动机器人的运动学解;最后进行了仿真研究. 仿真结果显示机器人的关节角度和绳长变化曲线十分平滑,末端的实际轨迹跟踪理想轨迹的 误差非常微小,说明建议的算法正确,绳驱动机器人运行理想,可以有效克服常规机器 人自重过大带来的负面影响.      

空间里的时间:微重力等环境下的生物节律研究

生物钟是地球上的生物为适应环境周期性变化经历长期演化而来的内在机制.在分子水平上受生物钟基因及其他相关基因的调节;在组织水平上,生物钟由主生物钟和外周生物钟组成.生物钟对于各种生物的生理、认知和行为等具有重要功能,是生物适应环境的决定因素之一.空间环境下的微重力、辐射、光照条件、社会性因素等与地面存在很大差异,这些因素均可能导致节律紊乱,影响生物的生理及环境适应性.因此,对地外生命的研究也应该考虑生物钟因素.对航天员而言,节律紊乱可引起睡眠障碍,并且对骨肌系统、神经系统、心血管系统及内分泌系统等造成不利影响,导致人的认知和工效水平下降.在未来空间生命探索以及航天员健康保障研究中,生物钟是一个不可忽视的重要因素.      

面向领域的仿真设计建模工具SIMDEMO

讨论了面向领域的仿真设计建模工具SIMDEMO的设计和实现.基于透明性、正交性、层次性的视图分解原理,对处于不同阶段、面向不同用户、涉及不同方面的系统模型采用多视图进行分解,建立了以多视图为核心理念的系统协同建模方法,给出了该建模方法下建模所需遵循的过程指导.针对领域模型描述、表示以及操作等多个方面对工具重构的需求,研究得到了基于元对象反射模型的工具架构;架构具有良好适应性,使得工具重构更灵活、简捷.对SIMDEMO的功能结构进行了简介,给出了系统实现方案.最后,将SIMDEMO与典型同类工具作了比较.