Forest parameter estimation by means of Monte-Carlo simulations with experimental considerations – Estimation of multiple reflections among trees depending on forest parameters

A method for estimation of forest multiple light reflections depending on forest parameters is introduced, based on Monte-Carlo simulations of photon transport with experimental considerations. The model is verified through experiments with two miniature forests, in which two types of small-sized trees with ellipsoid- and cone-shaped crowns are arranged in a grid array. The introduced method was confronted with experimental measurements and showed small deviations from the measured values. It was found that the simulation of three-dimensional photon trajectories allowed a reliable evaluation of multiple light reflections among trees. In addition, the multiple reflections among trees due to the changes of tree inter-distance, crown type and crown shape were clarified with the proposed method.     

250座级翼身融合无尾布局客机操稳特性设计研究

 翼身融合(BWB)飞翼布局是未来新一代客机的热点方案之一,然而由于没有常规尾翼,面临着稳定性和操纵性方面的困难。为此,在一架250座级BWB客机布局设计研究基础上,根据平衡、增稳和机动等要求,设计了操纵面配置方案;根据适航要求和电传飞机飞行品质要求设定增稳目标,并将其直接纳入特征结构配置要求中,通过前向通道修正响应类型,保证获得与飞行阶段相适应的响应特征和满意的飞行品质参数;为了提高安全性,在增稳控制设计基础上,在指令回路增设了姿态保护和限制模块。研究结果表明, 该设计方案能够提供较合适的稳定性和操纵性,控制增稳后具有满意的飞行品质,保护模块可达到预期效果。     

高压脉冲圆柱形阳极层霍尔等离子体加速器实验

描述了一台大尺寸高压脉冲阳极层霍尔等离子体加速器。对其磁场分布进行了分析,并进行了初步实验,包括放电特征、离子流引出特征、离子束形貌等特性,以验证大尺寸的圆柱形阳极层霍尔等离子体加速器在高功率条件下的运行状况。实验发现此霍尔等离子体加速器工作稳定,可以在较高的功率上运行（大于3kW）,电流利用率较高,可超出90%,工作电压范围很宽,可在300～2kV工作,束流汇聚性良好。     

硅微加速度计六自由度悬浮控制系统设计

六轴静电悬浮的硅微加速度计以其低量程、高分辨率和多轴集成等特点,在微小航天器的无拖曳控制、微重力测量等方面有着独特而重要的用途.本文针对外带梳齿式长方体检测质量的表头结构,依据带宽、量程、刚度等指标要求,经位移检测解耦变换与加力控制耦合变换后,分别设计出六轴稳定悬浮控制器.在地面大气环境下的仿真分析结果表明,阻尼最小的...     

非接触式静电电压测量仪校准方法研究

根据非接触式静电电压测量仪的工作原理,建立了一套非接触式静电电压测量仪校准系统.重点介绍了校准系统的组成和工作过程,以及决定校准系统测量准确度关键因素的标准平板电极的设计原则,并通过实验数据分析了标准平板电极的直径和边缘效应对测量结果的影响.最后以常用的非接触式静电电压测量仪EST101为例,根据校准装置测量不确定度主...     

某型飞机俯仰方位控制系统设计与仿真

为提高大迎角飞行状态下的战斗机等作战飞机控制系统的稳态精度,改善其控制系统的动态性能,对某型飞机俯仰方位控制系统结构进行改进设计。通过引入积分环节,将其俯仰方位控制系统由0型系统变为I型系统,提高了控制精度及抗干扰能力。通过合理配置俯仰方位控制系统控制规律传动比,对其动态性能也进行了有效改进。仿真结果显示：所设计的飞机俯仰方位控制系统结构合理,控制规律传动比配置恰当,对大迎角飞行状态下的飞机,其控制系统稳定性得到提高,其动、静态性能得到改善。     

Dust Environment Modelling of Comet 67P/Churyumov-Gerasimenko

Dust is an important constituent of cometary emission; its analysis is one of the major objectives of ESA’s Rosetta mission to comet 67P/Churyumov-Gerasimenko (C–G). Several instruments aboard Rosetta are dedicated to studying various aspects of dust in the cometary coma, all of which require a certain level of exposure to dust to achieve their goals. At the same time, impacts of dust particles can constitute a hazard to the spacecraft. To conciliate the demands of dust collection instruments and spacecraft safety, it is desirable to assess the dust environment in the coma even before the arrival of Rosetta. We describe the present status of modelling the dust coma of 67P/C–G and predict the speed and flux of dust in the coma, the dust fluence on a spacecraft along sample trajectories, and the radiation environment in the coma. The model will need to be refined when more details of the coma are revealed by observations. An overview of astronomical observations of 67P/C–G is given, because model parameters are derived from this data if possible. For quantities not yet measured for 67P/C–G, we use values obtained for other comets, e.g. concerning the optical and compositional properties of the dust grains. One of the most important and most controversial parameters is the dust mass distribution. We summarise the mass distribution functions derived from the in-situ measurements at comet 1P/Halley in 1986. For 67P/C–G, constraining the mass distribution is currently only possible by the analysis of astronomical images. We find that both the dust mass distribution and the time dependence of the dust production rate of 67P/C–G are those of a fairly typical comet.     

满足一等量块检定要求的接触式激光量块干涉仪

最新研制的接触式激光量块干涉仪主要用于测量一、二等量块的中心长度，其长度测量不确定度达到（0.02 0.2L)μm。文中介绍了其工作原理、测量不确定度分析，给出了量块测量的验证数据。     

Pickup Ions and Cosmic Rays from Dust in the Heliosphere

The combination of recent observational and theoretical work has completed the catalog of the sources of heliospheric Pickup Ions (PUIs). These PUIs are the seed population for Anomalous Cosmic Rays (ACRs), which are accelerated to high energies at or beyond the Termination Shock (TS). For elements with high First Ionization Potentials (high-FIP atoms: e.g., H, He, Ne, etc.), the dominant source of PUIs and ACRs is from neutral atoms that drift into the heliosphere from the Local Interstellar Medium (LISM) and, prior to ionization, are influenced primarily by solar gravitation and radiation pressure (for H). After ionization, these interstellar ions are pickup up by the solar wind, swept out, and are either accelerated near the TS or beyond it. Elements with low first ionization potentials (low-FIP atoms: e.g., C, Si, Mg, Fe, etc.) are also observed as PUIs by Ulysses and as ACRs by Wind and Voyager. But the low-FIP composition of this additional component reveals a very different origin. Low-FIP interstellar atoms are predominantly ionized in the LISM and therefore excluded from the heliosphere by the solar wind. Remarkably, a low-FIP component of PUIs was hypothesized by Banks (J. Geophys. Res. 76, 4341, 1971) over twenty years prior to its direct detection by Ulysses/SWICS (Geiss et al., J. Geophys. Res. 100(23), 373, 1995) The leading concept for the generation of Inner Source PUIs involves an effective recycling of solar wind on grains near the Sun, as originally suggested by Banks. Voyager and Wind also observe low-FIP ACRs, and a grain-related source appears likely and necessary. Two concepts have been proposed to explain these low-FIP ACRs: the first concept involves the acceleration of the Inner Source of PUIs, and the second involves a so-called Outer Source of PUIs generated from solar wind interaction with the large population of grains in the Kuiper Belt. We review here the observational and theoretical work over the last decade that shows how solar wind and heliospheric grains interact to produce pickup ions, and, in turn, anomalous cosmic rays. The inner and outer sources of pickup ions and anomalous cosmic rays exemplify dusty plasma interactions that are fundamental throughout the cosmos for the production of energetic particles and the formation of stellar systems.     

民航安全文化变革探析

民航安全文化变革是民航安全文化自我创新、建设发展的重要途径。其变革方式有渐进性变革与突发性变革、主动变革与被动变革之分;其变革步骤主要按照PDCA循环实施;其变革规律主要是由浅层到深层、无序到有序、量变到质变。