Distinct EUV minimum of the solar irradiance (16–40 nm) observed by SolACES spectrometers onboard the International Space Station (ISS) in August/September 2009

In the field of terrestrial climatology the continuous monitoring of the solar irradiance with highest possible accuracy is an important goal. SolACES as a part of the ESA mission SOLAR on the ISS is measuring the short-wavelength solar EUV irradiance from 16–150 nm. This data will be made available to the scientific community to investigate the impact of the solar irradiance variability on the Earth’s climate as well as the thermospheric/ionospheric interactions that are pursued in the TIGER program. Since the successful launch with the shuttle mission STS-122 on February 7th, 2008, SolACES initially recorded the low EUV irradiance during the extended solar activity minimum. Thereafter it has been observing the EUV irradiance during the increasing solar activity with enhanced intensity and changing spectral composition. SolACES consists of three grazing incidence planar grating spectrometers. In addition there are two three-signal ionisation chambers, each with exchangeable band-pass filters to determine the absolute EUV fluxes repeatedly during the mission. One important problem of space-borne instrumentation recording the solar EUV irradiance is the degradation of the spectrometer sensitivity. The two double ionisation chambers of SolACES, which could be re-filled with three different gases for each recording, allow the recalibration of the efficiencies of the three SolACES spectrometers from time to time.     

The Radio Observatory on the Lunar Surface for Solar studies

The Radio Observatory on the Lunar Surface for Solar studies (ROLSS) is a concept for a near-side low radio frequency imaging interferometric array designed to study particle acceleration at the Sun and in the inner heliosphere. The prime science mission is to image the radio emission generated by Type II and III solar radio burst processes with the aim of determining the sites at and mechanisms by which the radiating particles are accelerated. Specific questions to be addressed include the following: (1) Isolating the sites of electron acceleration responsible for Type II and III solar radio bursts during coronal mass ejections (CMEs); and (2) Determining if and the mechanism(s) by which multiple, successive CMEs produce unusually efficient particle acceleration and intense radio emission. Secondary science goals include constraining the density of the lunar ionosphere by searching for a low radio frequency cutoff to solar radio emission and constraining the low energy electron population in astrophysical sources. Key design requirements on ROLSS include the operational frequency and angular resolution. The electron densities in the solar corona and inner heliosphere are such that the relevant emission occurs at frequencies below 10 MHz. Second, resolving the potential sites of particle acceleration requires an instrument with an angular resolution of at least 2°, equivalent to a linear array size of approximately 1000 m. Operations would consist of data acquisition during the lunar day, with regular data downlinks. No operations would occur during lunar night.     

智能太阳翼动力学建模与模态分析

研究柔性航天器的动力学与控制问题时,通常需要利用柔性附件的模态信息。为获取航天器的高精度姿态控制,必须解决柔性附件的振动抑制问题。配置压电传感/作动器是解决太阳翼振动控制的有效手段。针对基板表面粘贴压电传感/作动器的太阳翼,基于一阶剪切变形层板理论,建立了包含机电耦合效应对结构刚度贡献的有限元模型,并在连接机构等效梁单元中引入了轴向载荷。利用假设剪切应变方法解决了一阶剪切变形层板理论的剪切闭锁问题。仿真结果表明:太阳翼的动力学特征随压电传感/作动器配置方式的改变而改变;连接架轴向载荷可以大幅提高太阳翼的侧摆振动频率;给压电作动器施加控制电压可以增加太阳翼的结构阻尼。     

编队卫星空间状态与星间基线的建模与分析

针对编队卫星任务中起重要作用的星间基线指标,在考虑精度需求的基础上对用于确定星间基线的空间状态量进行了选择,建立了空间状态量与星间基线的关联数学模型,提供了误差分析方法,仿真给出了一定场景设置下的精度影响因子等指标以定量刻画二者之间的误差传播关系。基线长度仅与编队卫星的相对空间状态有关,而基线姿态角还与主星的绝对姿态有关;且由卫星空间状态得到星间基线的过程中误差放大。     

太阳风扰动对极光电急流和环电流指数的影响

利用WIND卫星的太阳风观测数据和地磁活动指数, 研究了太阳风扰动对环电流SYM-H指数, 西向极光电急流AL指数和东向极光电急流AU指数的影响. 结果表明, 太阳风动压增长和减少能够同步或延迟引起地磁活动指数的强烈扰动, 其包括环电流指数的上升, 西向极光电急流指数的下降和东向极光电急流指数的上升. 太阳风动压的突然剧烈增加还能够触发超级亚暴和大磁暴. 太阳风动压脉冲引起的地磁效应具有复杂的表现形式, 这说明太阳风动压脉冲的地磁效应不仅与太阳风动压脉冲大小和持续时间有关, 还与磁层本身所处的状态有关. 时间尺度较长, 消耗能量较大的磁暴只有大的持续时间较长的太阳风动压脉冲才能激发.      

空管系统中双机热备份管理的设计与实现

在空管关键系统中,一些双机热备份子系统由于系统检测容错软件本身存在出错的可能性,使得双机热备份系统的可靠性降低。本文介绍了空管系统中基于代理检测的应用级双机热备份系统的设计原理及其具体实现。     

矢量控制的无刷交流电动机调速系统仿真

本文介绍交流无刷电动机调速系统的仿真方法,知仿真数学模型的建立,速度调节系统控制策略的确定及仿真ＳＩＭＵＬＩＮＫ实现等。本文也给出了一个基于仿真结果设计的实际调速系统。     

热变形Pr-Fe-B-Cu磁织构的形成机制及〔006〕织构的获得

本文提出Ｐｒ－Ｆｅ－Ｂ－Ｃｕ热压历程判据的计算式：ｆ（Ｔ，ε）＝Ｔ２２１１５３９．９ｌｇε＋１８９５７４８８。判据认为：在变形温度≥１１７３Ｋ时，ｆ（Ｔ，ε）＞１，则热压磁体的其它峰强比较小，Ｉ（００６）／Ｉ（１０５）≥０．６０；Ｉ（００６）／Ｉ（１０５）与变形量ε之间存在如下关系式：Ｉ（００６）／Ｉ（１０５）＝０．９８３ε＋０．４６５；分析了｛１０５｝成为主滑移系的原因。在Ｔ＜１１７３Ｋ，ｆ（Ｔ，ε）＞１时，首次得到热压Ｐｒ－Ｆｅ－Ｂ－Ｃｕ的〔００６〕织构，并讨论了〔００６〕织构的形成原因。当ｆ（Ｔ，ε）≤１，热压磁体均破断开裂，形成不完善的〔１０５〕织构。在热变形中，Ｐｒ２Ｆｅ１４Ｂ均存在严重的点阵畸变、原子错位，热处理后可恢复正常。     

用现代谱估计法实现导弹系统仿真模型的高可信度确认

本文概述导弹仿真模型的确认方法和各自的优缺点及应用范围。分析了导弹系统仿真过程输出序列的特点,并根据现代谱估计方法对短序列、低信噪比序列进行谱估计时分辩力高的特点,提出了一种导弹系统仿真模型有效性确认的新方法,并结合某型号半实物仿真过程给出应用结果。     

高置信度验模方法及若干问题探讨

本文论述导弹系统仿真建模、验模及一体化研究问题，概述建模的主要内容，提出验模的一般观点，分析现有验模方法用于导弹系统仿真模型验证时的困难和局限性，并提出高置信度验模方法的基本特征和方法研究的技术途径。同时，就如何保证仿真模型验证结果具有高的置信水平所关联的问题进行探讨。