激光技术在高技术国防战争中的应用

介绍激光技术的基本含义以及激光技术在新军事应用中的分类,并结合我军的军事战略,从激光侦查技术、激光对抗与激光干扰技术、激光模拟训练技术以及激光武器四个方面对激光技术在高技术国防战争中的应用进行分析,最后结合装甲装备,介绍激光技术在观瞄系统中的具体应用。     

Compensation of time-variable magnetic moments for a precise attitude control in nano- and micro-satellite missions

Theses days, many nano- and micro-satellites are applied to several astronomy and remote sensing missions. In order to achieve mission requirements, these satellites must control the attitude precisely. A magnetic disturbance is one of the dominant sources of attitude disturbances. Therefore, this disturbance should be canceled in-orbit or on the ground to achieve the attitude strict requirements. This paper presents the effect of the magnetic disturbance to the attitude in nano- and micro-satellite missions and the sources of the residual magnetic moment of the satellites, which causes the magnetic disturbance. Then, the paper proposes a method to compensate the residual magnetic moment both in-orbit and in the design phase of the satellites. The research also focused on a time-varying residual magnetic moment. Finally, the method is applied to a micro-astrometry satellite as an example.     

Study of the ionosphere during a magnetospheric storm using data on the ground and in space

For the magnetospheric storm of May 14–16, 1997 geophysical data of satellites DMSP and IMP-8 are compared with data of radio propagation on the high-latitude HF radio path of Heiss Island – St. Petersburg and data from European ionosondes. Peculiarities of variations of the operational frequencies range MOF–LOF (maximum and lowest observed frequencies) on the path were considered. The range has been determined by the method of oblique ionospheric sounding (OIS). The latter is more informative for observations during a magnetic storm compared to the vertical sounding method. Nevertheless, an analysis of variations of the critical frequency of the ionospheric F2 layer from the chain of European ionosondes was carried out. For interpretation of results, data of magnetospheric parameters, AE-indexes and riometer data were used. The variations of both frequency range on the path and critical frequencies of the F2 layer through the ionosondes chain during the disturbed period had certain regularities of behaviour. These regularities are being explained from the physical point of view. The analysis of the satellite DMSP data has showed that a magnetospheric disturbance causes displacement equatorward of precipitation and some growth of its width and energy.     

Study of TEC changes during geomagnetic storms occurred near the crest of the equatorial ionospheric ionization anomaly in the Indian sector

GPS satellites data obtained at Bhopal (23.16° N, 77.36° E, geomagnetic latitude 14.23° N) India were analyzed to study the TEC changes during several geomagnetic storms (−300 nT < Dst < −50 nT) occurred in 2005–2007. We had segregated the storms according to the Dst value, i.e. moderate storms (−100 nT < Dst ? −50 nT), strong storms (−150 nT < Dst < −100 nT), and severe storms (Dst less than −150 nT). Total of 21 geomagnetic storms (10 moderate, 9 strong, 2 severe) are considered for the present study. Deviation in vertical total electron content (VTEC) during the main phase of the storm was found to be associated with the prompt penetration of electric field originated due to the under-shielding and over-shielding conditions for almost all geomagnetic storms discussed in this paper. For most of the storms VTEC shows the positive percentage deviation during the main phase while it shows positive as well as the negative deviation during the recovery phase of the storms. The −80% deviation in VTEC was found for geomagnetic storm occurred on July 17, 2005 and the negative trend continued for recovery phase of the storm. This was mainly due to the thermospheric composition changes by Joule heating effect at auroral latitudes that generate electric field disturbance at low latitudes. Traveling ionospheric disturbances (TIDs) were responsible for the formation of wave like nature in VTEC for the storms occurred on May 15, 2005, whereas it was not observed for storm occurred on August 24, 2005.     

一种加速度干扰下的稳定被动定位跟踪算法

在研究一种具有误差自动解耦的观测域滤波的目标跟踪算法和自适应渐消EKF算法的基础上,提出一种匀速运动模型下,基于观测域的自适应目标跟踪算法。使用实测GPS导航数据进行数字仿真,结果表明：观测域的自适应目标跟踪算法在加速度扰动下,稳定性优于观测域滤波算法。     

弹上计算机自主抗干扰技术研究

分析了干扰作用机理 ,干扰对弹上计算机状态的影响 ,研究了计算机自主抗干扰技术 ,包括状态偏差的检测方法和正确状态的记录和恢复方法等 ,并给出了应用实例。     

一种小天体探测器绕飞轨道主动抗扰控制方法

针对小天体绕飞探测过程中,探测器受到的非球形引力摄动及太阳光压等多源扰动问题,结合绕飞探测的周期性特点,提出一种小天体探测器绕飞轨道主动抗扰控制方法。首先,通过迭代学习控制对小天体探测器受多源扰动影响产生的误差进行抑制,然后设计扰动观测器估计系统总扰动,构造自适应律实时估计扰动上界,进而设计控制律对总扰动进行主动补偿。最后以243Ida作为目标天体进行绕飞探测仿真分析,结果表明该控制方法能更加有效地提高小天体探测器的轨道跟踪控制精度。     

基于ADRC的航空发动机限制保护器设计

发动机限制保护器在航空发动机运行过程中对特定的被限制量进行实时监控,在其超出安全范围时实施限制,实现对航空发动机的保护.将自抗扰技术用于限制保护控制器设计,利用自抗扰控制器的扩张观测器,动态估计未知扰动和系统特性,对实际控制量进行反馈补偿,实现超限后的快速保护,提高了发动机的安全性.仿真结果表明:所设计的自抗扰限制保护控制器能将超限偏差有效转化为对主回路指令的修正,综合控制系统响应速度快,达到了限制保护的目的.     

地磁扰动期间低轨目标轨道预报的误差修正

针对地磁扰动期间大气密度变化造成的低轨目标较大的轨道预报误差,提出一种根据POES卫星观测的极光能量注入数据改进短期轨道预报的方法。分析表明CHAMP卫星的沿迹大气密度及轨道衰减与极光能量注入具有较好的相关性。通过线性回归方法,建立轨道半长轴衰减及阻力调制系数的修正公式,并使用修正后的阻力调制系数取代两行元(TLE)中的该系数带入SGP4模型进行位置预报。该方案考虑了外推过程中地磁扰动引起的大气密度响应,能更准确地反映外推过程中大气阻力对轨道的影响。将其应用到2008年CHAMP卫星和国际空间站的轨道预报中,结果表明,半长轴和位置的预报误差可分别降低50%和30%左右。进一步对不同年份、不同轨道高度的目标进行了预报误差修正的分析,验证了该方法的普适性。     

幅值锁定型超流体陀螺模糊自抗扰控制系统设计

针对幅值锁定型超流体陀螺中热相位注入存在的温升延迟和热噪声影响陀螺系统测量精度和稳定性的问题,提出一种基于模糊自抗扰的超流体陀螺控制系统设计方法。首先建立超流体陀螺的数学模型;分析热相位注入引入的温升延迟和未知热噪声对系统敏感精度和稳定性的影响机理。在此基础上,设计集微分跟踪器、扩张状态观测和非线性反馈控制律于一体的自抗扰控制器,并进一步采用模糊推理实现非线性组合的比例和微分系数的自适应调整。最后利用Maltlab/Simulink进行仿真校验。仿真结果表明：该控制方法能够抑制未知噪声和温升延迟对系统的影响,对工作点实现良好的锁定,有效地提高了陀螺系统的测量精度和稳定性。