外辐射带动态演化的粒子模拟研究

运用计算机实验方法即三维电磁粒子模拟方法初步研究了暴时扰动情况下外辐射带粒子环境的动态演化特性。模拟计算了暴时辐射带粒子环境的演化情况。模拟计算结果显示，高能质子、电子注入午辐射滞后，两者一方面沿磁力线做弹跳运动，向高纬扩展，部分注入质子和电子沉降于南北两极区域；另一方面，注入质子和电子还经历顺时针和逆时针方向的漂移运动，粒子能量越大，漂移速度越快。暴时多次注入引起整个辐射带粒子能量的大幅增强；粒子注入颗次和强度越大，辐射带粒子通量增幅越大。本项研究为开发研制完整的辐射带动态模式积累了有益的经验。     

Ray Structure of the Coronal Streamer Belt and Its Manifestation as Sharp Large Peaks of Solar Wind Plasma Density at the Earth''''s Orbit

The white-light corona calibrated data with processing level L1 from the LASCO-C2/SOHO instrument, and data from the Wind spacecraft with one-hour and one-minute time resolution on quasi-stationary slow (v between 300-450 km/s at the Earth's orbit) the Solar Wind (SW) parameters in the absence of sporadic SW streams are examined. Within distances from the Sun's center less than R in the range of 20-30 Rs, (Rs, the solar radius), slow wind is known as the streamer belt, and at larger distances it is called the He-liospheric Plasma Sheet (HPS). It is shown that the streamer belt comprises a sequence of pairs of rays. In general, ray brightnesses in each pair can differ, and the magnetic field is oppositely directed in them. The neutral line of the radial magnetic field of the Sun runs along the belt between the rays of each of the pairs. The area in which the streamer belt intersects the ecliptic plane and which lies at the central meridian, will be recorded at the earth's orbit with a time delay of 5-6 days, in the form of one or several peaks with Nmax> 10cm-3. Furthermore, the simplest density profile of the portion of the HCS has the form of two peaks of a different or identical amplitude . The such a profile is observed in cases where the angle of intersection of the streamer belt with the ecliptic plane near the Sun is sufficiently large, i.e. close to 90°. The two-ray structure of the cross-section of the streamer-belt moves from the Sun to the Earth, it retains not only the angular size of the peaks but also the relative density variations, and the position of the neutral line (sector boundary) in between. At the Earth's orbit the ray structure of the streamer belt provides the source for sharp (i.e. with steep fronts of a duration of a few minutes or shorter) solar wind plasma density peaks (of a duration of several hours) with maximum values Nmax> 10cm-3.     

Working Group 3 Report: Coronal Hole Boundaries and Interactions with Adjacent Regions

Summarized below are the discussions of working group 3 on "Coronal hole boundaries and interactions with adjacent regions" which took place at the 7th SOHO workshop in Northeast Harbor, Maine, USA, 28 September to 1 October 1998. A number of recent observational and theoretical results were presented during the discussions to shed light on different aspects of coronal hole boundaries. The working group also included presentations on streamers and coronal holes to emphasis the difference between the plasma properties in these regions, and to serve as guidelines for the definition of the boundaries. Observations, particularly white light observations, show that multiple streamers are present close to the solar limb at all times. At some distance from the sun, typically below 2 R, these streamers merge into a relatively narrow sheet as seen, for example, in LASCO and UVCS images. The presence of multiple current sheets in interplanetary space was also briefly addressed. Coronal hole boundaries were defined as the abrupt transition from the bright appearing plasma sheet to the dark coronal hole regions. Observations in the inner corona seem to indicate a transition of typically 10 to 20 degrees, whereas observations in interplanetary space, carried out from Ulysses, show on one hand an even faster transition of less than 2 degrees which is in agreement with earlier Helios results. On the other hand, these observations also show that the transition happens on different scales, some of which are significantly larger. The slow solar wind is connected to the streamer belt/plasma sheet, even though the discussions were still not conclusive on the point where exactly the slow solar wind originates. Considered the high variability of plasma characteristics in slow wind streams, it seems most likely that several types of coronal regions produce slow solar wind, such as streamer stalks, streamer legs and open field regions between active regions, and maybe even regions just inside of the coronal holes. Observational and theoretical studies presented during the discussions show evidence that each of these regions may indeed contribute to the solar slow wind. This revised version was published online in June 2006 with corrections to the Cover Date.     

木星环绕探测任务中的内带电风险评估

木星拥有类似地球辐射带的辐射带结构,其辐射带质子通量是地球的10倍,高能电子通量比地球高2~3个数量级,且最高能量可达1 Ge V。因此木星探测任务的抗辐射设计是任务成功的关键。选择3种不同倾角大椭圆探测轨道,仿真分析了2种介质在变化能谱下的内带电过程。仿真结果表明,对于环氧树脂(Fr4),由于电阻相对较小,电子通量较大的近木点的充电电荷,会在远离辐射带时泄放,其最大充电电场取决于近木点的电子通量;对于聚酰亚胺(Kapton),由于电阻相对较大,充电电荷不能及时泄放,不同轨道间电荷逐渐累计,最大电场不断增加。另外,环木轨道倾角越大,越有利于降低充电电场。和地球GEO轨道相比,不同电阻介质在环木轨道的充电差异相对地球GEO轨道较小。     

SiC材料机器人砂带磨削系统设计及试验研究

通过分析SiC材料的加工特点及难点,针对SiC材料成型后加工易产生崩边、开裂等问题,设计并搭建了机器人砂带柔性磨削系统,开展了相关试验研究工作。结果表明, 所搭建的砂带磨削系统可有效避免SiC材料加工过程中的崩边、开裂问题。     

航空发动机叶片机器人精密砂带磨削研究现状及发展趋势

航空发动机叶片的型面精度及表面完整性对其疲劳寿命和气流动力性等影响巨大。机器人砂带磨削由于其灵活性好、易于调度、通用性强等特点成为提高叶片表面完整性的有效加工方法之一,但是工业机器人一般仅适用于粗加工,而对于半精加工以及精加工,提高机器人的定位精度是决定加工质量的关键问题。因此,对航空发动机叶片机器人砂带磨削研究现状进行归纳总结,为实现叶片精密磨削提供参考。首先,对叶片机器人砂带磨削系统的组成和结构形式进行了论述,从磨削接触廓形、材料去除规律和表面完整性等方面对砂带磨削机理进行了分析;其次,分别从基于CAD模型、数学模型和人工知识学习三方面总结了叶片机器人砂带磨削轨迹规划方法;然后,对叶片机器人砂带磨削运动控制技术研究进行了介绍,并分析了叶片机器人砂带磨削系统及集成技术;最后,对航空发动机叶片机器人砂带磨削研究现状进行了总结,在此基础上对其发展趋势进行了分析。     

建设“郑州空中丝绸之路试验区”的战略思路

"一带一路"是我国对外开放和构建现代开放型经济体系的主体战略,全国各地都在探索"一带一路"试验区建设,河南省应发挥战略叠加、经济大省、国际枢纽、总书记指示等独特优势,差异化构建"郑州空中丝绸之路试验区",以"郑州航空港区"为核心打造自由贸易港,以"郑汴港金三角新区"为主体打造国家级城市新区和自由贸易试验区,以"郑州1+5同城化"为支撑打造"黄河大湾区"国际产业科创中心,以"五龙、五通、五城"为重点,建设世界一流空中丝绸之路试验区、世界一流枢纽型中心城市、世界一流内河大湾区。     

永磁同步电机弱磁与过调制控制策略研究

在前人研究的基础上,提出了一种提升永磁同步电机(PMSM)高速带载能力的控制策略。该控制策略能克服电机在最高转速时无法带载的弱点,可靠性高、易于实现。实现该控制策略的算法包含PMSM的弱磁控制和电压空间矢量的过调制控制,使电机能宽范围带载调速。为验证该控制策略,建立了内置式永磁同步电机(IPMSM)的仿真模型,搭建了试验平台,并进行了仿真和试验研究,验证了该控制策略的可行性和有效性。     

机器人修形磨削工具坐标系的精确标定方法

针对目前机器人修形磨削系统中接触轮姿态标定精度低影响磨削精度的问题,提出了一种实验测量的工具坐标系标定方法,姿态标定精度达0.05°.首先总结了通用静态标定法的不足之处,提出了新标定方法的构思并且理论证明了该方法的正确性.介绍了实验系统的组成,并在机器人砂带磨削系统上做了磨削实验.采集了磨削处的实验数据,分析实验数据,获得接触轮的实际偏转角,把偏转角补偿到磨削路径的工具坐标系上,最后完成了工具坐标系补偿后的重复性实验,证明了该方法的可行性和准确性.     

A noise attenuation method for medium-energy electron measurements in the radiation belt

From the viewpoint of plasma particle measurements in the radiation belt, background noise is a serious problem. High-energy particles penetrating the sensor shielding generate spurious signals, and their count rate often can be comparable to the true signals. In order to attenuate such background noise during medium-energy (5–83 keV) electron measurements, we propose the double energy analyses (DEA) method. DEA is conducted by a combination of an electrostatic analyser (ESA) and avalanche photo-diodes (APDs); ESA and APD independently determine the energy of each incoming particle. By using the DEA method, therefore, the penetrating particles can be rejected when the two energy determinations are inconsistent; spurious noise are caused only when the deposited energy at an APD is by chance consistent with the measured energy by ESA. We formulate the noise count rate and show the advantage of DEA method quantitatively.