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1.
    
电力线谐波辐射(PLHR)作为一种人为的电离层电磁环境污染源被广泛认可,其对电离层状态的影响亟待研究。基于DEMETER卫星高能粒子探测器(IDP)的数据,采用PLHR事件自轨道和发生前后重访轨道综合分析的方法,研究了中国电离层中发现的72例PLHR事件发生前后电离层高能电子投掷角、低中高3个能带的电子通量的影响。结果表明,在PLHR发生前极少数事件出现了投掷角增大的现象,且低能带的电子通量倾向于减小的趋势。这可能是PLHR产生的影响,也可能是由于电离层高能电子状态的这种变化导致PLHR更容易被探测到。  相似文献   

2.
    
多电/全电飞机的发展使得机电作动系统(EMA)逐渐应用于飞机舵面的作动,其故障模式和故障影响问题是适航审查的重点。为解决机电作动系统中非指令振荡信号导致的故障模式及故障影响不明确的问题,分析了振荡信号的产生机理、产生位置及表现形式,对变频率、变幅值的振荡信号在机电作动系统中的故障传播和影响展开研究。结果表明:系统架构会改变振荡信号波形,传感器输出振荡信号对系统的故障影响最大,系统舵偏角输出与振荡信号同频率变化,且频率在0.2~3 Hz、8~10 Hz的振荡信号会引发电磁转矩与舵偏角不可接受的振荡,振荡信号幅值影响系统跟踪指令的速度。  相似文献   

3.
    
为了降低有源传感器在获得目标持续量测时被敌方截获的风险,提出一种多传感器协同跟踪与辐射控制的调度算法。该算法首先采用辐射度影响(ELI)衡量传感器辐射,将目标跟踪与辐射控制过程建立为部分可观马尔可夫决策(POMDP)过程。然后以隐马尔可夫模型(HMM)滤波器更新传感器辐射状态、推导长时辐射风险,以无迹卡尔曼滤波(UKF)更新目标状态、估计跟踪精度。最后考虑跟踪任务需求,构建精度约束下辐射控制的长时调度模型,并将该长时调度问题转化为决策树寻优问题,给出决策树节点次优下界值,采用改进分支定界技术(IB&B)快速求解最优调度序列。仿真结果验证了本文算法的有效性。  相似文献   

4.
张轩谊 《空间科学学报》2022,42(6):1129-1136
太阳紫外辐射是临近空间能量输入的主要来源之一,对其在中层大气的辐射特性进行研究,是研究临近空间大气成分与密度变化、光化学反应以及动力学过程的重要基础。依托“鸿鹄”临近空间探测专项计划,利用MODTRAN5辐射传输模型及卫星实测数据,模拟并对比中国11个主要地形区上空临近空间(20~50 km)紫外辐射(200~400 nm)垂直分布和季节演变的异同,计算了臭氧含量、太阳天顶角和日地距离等关键因素对辐射强度的影响。结果表明,各地形区的辐射流量垂直分布廓线和年较差垂直分布廓线较为一致,在地理位置上毗邻的地区辐射特性及季节演变较为接近,但在太阳紫外的不同波段之间区别较大。研究成果为临近空间探测实验提供了数据支撑,为大气反演等相关领域提供参考。   相似文献   

5.
    
为了降低极化敏感阵列(PSA)的应用成本,优化极化信息的利用效率,提高导向矢量失配条件下的滤波性能,提出了极化敏感辅助阵列(APSA)模型和基于二相编码信号非圆特征恢复的波束形成算法。在单极化线阵的基础上对部分阵元进行双极化改造,构成APSA;根据接收信号矢量的协方差阵和共轭协方差阵,按照非圆率最大准则,对构造的新协方差阵进行特征分解以确定权矢量,进而完成数字波束形成。详细分析了阵列模型的性能,并讨论了最小方差无失真响应(MVDR)算法和特征子空间投影(EP)算法。仿真结果表明,二相编码的非圆特征恢复算法不受导向矢量误差的影响,在阵列模型的基础上有主瓣干扰对抗能力,鲁棒性强。  相似文献   

6.
  总被引:1,自引:0,他引:1  
为从受谐波和随机噪声干扰的振动信号中提取出故障冲击成分,融合四大基本形态学算子提出了改进形态滤波方法--平均组合差值形态滤波(ACDIF)方法,同时与固有时间尺度分解(ITD)相结合,并将ITD-ACDIF方法应用到滚动轴承的故障诊断中。首先,对轴承振动信号进行ITD分解得到一系列旋转分量(PRC);然后,以峭度为准则筛选出含故障信息丰富的有效PRC,对每个有效分量进行ACDIF滤波提取冲击成分进行信号重构;最后,利用频谱分析提取重构信号中的故障特征。数值仿真和轴承故障振动信号的试验结果表明,本文方法可有效滤除谐波干扰,提取强背景噪声下的冲击故障特征,实现设备的故障诊断。  相似文献   

7.
  总被引:1,自引:1,他引:0  
提出利用全球导航卫星系统反射信号的干涉方法(GNSS-IR)进行测高。深入分析全球导航卫星系统反射信号的多径信号模型(GNSS-MR),在此基础上提出单天线测高模型,旨在获取多径信号信噪比(SNR)频率信息,从而反演出高度信息。Lomb-Scargle(LS)谱分析方法是单天线测高模型中常用的频率提取方法;提出了基于解析模型拟合的方法对多径信号信噪比数据提取频率,同样可以准确获取频率信息,从而反演出天线到地面的高度。在此基础上,讨论了单天线测高的最大测量高度和接收机需要满足的最小输出率。由实验数据分析得出:传统LS谱分析方法和拟合法在反演效果最优时,即LS谱分析方法在高度角上限为17°时,均方根误差为0.028 75 m;拟合法在高度角上限为21°时,均方根误差为0.024 85 m。通过比较不同高度角上限的均方根误差,可以获得最优化的高度反演条件,同时也表明了拟合法的可行性。  相似文献   

8.
  总被引:1,自引:1,他引:0  
随着全球导航卫星系统反射信号(GNSS-R)的提出,其在海冰检测领域的应用也越来越广泛。北斗地球同步轨道(GEO)卫星的角速度较小且仰角变化仅有3°~4°,因此在相同观测地点其镜面反射点的空间位置非常稳定,可以提高特定区域海冰检测的时间分辨率。对在中国渤海湾进行的2次岸基海冰检测实验(2015年1月24日和2016年1月30日至2月4日)进行分析,验证了北斗GEO B1反射信号对沿岸海冰进行长时间连续检测的可行性。第1个实验结果显示海冰密集度与2颗GEO卫星C01和C03的极化比值结果具有相关性;第2个实验结果显示3颗GEO卫星C01、C02和C03检测的海冰极化比值与大气温度存在正相关关系,其中C01、C02和C03的极化比值与大气温度的相关值分别为0.61、0.72和0.57。  相似文献   

9.
    
针对功耗和工作频率对22 nm FDSOI背偏和28 nm体硅体偏电路的偏置能力进行对比和分析。以带有4级分频电路的65级环阵(RO)为例进行后仿真,后仿真结果表明,利用背偏技术的22 nm FDSOI环阵的输出频率可在57.8~206 MHz的范围内进行调节,相应的工作电流变化范围为24.4~90.4 μA;而利用体偏技术的28 nm体硅环阵的输出频率调节范围则为92.8~127 MHz,对应的工作电流变化范围为67.8~129 μA。对22 nm FDSOI工艺的环阵进行了实测,实测结果与仿真结果一致。分析认为,在功耗和性能2个方面,22 nm FDSOI电路的背偏调节能力优于28 nm体硅电路的体偏调节能力。  相似文献   

10.
    
共因失效(CCF)打破了系统内组件失效的独立性假设,会对系统特别是多阶段任务系统(PMS)的可靠性评估产生显著影响。针对多阶段任务系统中随机共因失效(PCCF)对任务可靠性的影响问题,对共因事件之间的关系进行分析,利用贝叶斯理论扩展了共因事件的概率模型,使其适用于互斥、相互独立和统计相关等多种统计关系。在此基础上提出了综合应用二元决策图(BDD)和马尔可夫(Markov)模型的模块化建模分析方法。首先,利用故障树对任务过程建模;然后,在考虑共因失效的情况下采用BDD和Markov模型分别计算系统中静态模块和动态模块;再次,由全概率公式计算任务可靠性;最后,以卫星首次转轨过程为对象,验证了方法的有效性,并通过与已有案例的对比,分析了共因失效对任务可靠性的影响。  相似文献   

11.
研究了利用DEMETER卫星电磁场探测数据辨识电力线谐波辐射(PLHR,Power Line Harmonic Radiation)事件的方法,探讨了我国空间中PLHR事件的特点.通过采用时频分析和Welch功率谱估计法分析了2005-2010年6年我国空间中的全部卫星电场强度探测数据,共发现151例PLHR事件,给出了PLHR事件的统计分析和典型实例.结果表明我国空间PLHR事件的频率分布在1 000~4 500 Hz之间,多为50 Hz的奇数倍,间隔为50/100 Hz.PLHR事件与我国电网发展和变化有密切关系,与地磁活动水平无关,呈现出昼夜差异和季节差异.最后给出了影响PLHR事件探测的可能因素.  相似文献   

12.
MLR events and associated triggered emissions observed by DEMETER   总被引:1,自引:0,他引:1  
This paper gives an overview of different sets of new Magnetospheric Line Radiation (MLR) observed by the satellite DEMETER. Different types of emissions have been observed: emissions called Power Line Harmonic Radiation (PLHR) with frequency lines exactly separated by 50/100 or 60/120 Hz, emissions with frequency lines not exactly separated by 50/100 or 60/120 Hz and drifting in frequency (MLR). By comparison with past observations one can say that some MLR events are due to man-made PLHR which may suffer a non-linear gyro-resonant interaction at the magnetic equator. It is also shown that periodic emissions are very often associated with the MLR. In this case the origin of these waves is natural. The lines are produced by the periodicity and the frequency band limits of the individual elements which causes the appearance of lines on the spectrograms. Finally the paper shows that MLR can trigger emissions.  相似文献   

13.
The Chinese Meridian Space Weather Monitoring Project (Meridian Project) is a ground-based geospace monitoring chain in China. It consists of 15 ground-based observation stations located roughly along 120°E longitude and 30°N latitude. In recent two years, using data from the Meridian Project, significant progress has been made in space weather and space physics research. These advances are mainly in four aspects:regional characteristics of space environment above China or along 120°E meridian line, coupling between space spheres at different heights and different physical processes, space weather disturbance and its propagation along the meridian chain, and space weather effects on ground technical facilities.   相似文献   

14.
位于低纬地区的印度同时测量了短波紫外辐射与臭氧含量,表明臭氧含量下降3%,短波紫外辐射通量(290nm)上升35%.但这个数值大于以往理论预期的数值.本文给出一个简单公式,这个公式描述了臭氧含量的变化与相应的紫外辐射变化之间的关系,用此公式计算得出的结果与印度测得的结果相符,很好地解释了低纬地区的印度测量的臭氧涨落与其相应的短波长紫外辐射变化之间的关系.   相似文献   

15.
利用Cluster,TC-1以及中国和欧洲在中低纬六个地面台站的数据,分析了2004年10月22日1700-1930 UT发生的三次BBF事件过程中地面和近地空间磁场脉动的特性.这三次BBF事件都发生在地磁活动的平静时期.结果发现,有两次平静时期的BBF确实对应着阻尼型Pi2脉动,并且脉动的特征与以前观测结果中的特征类似.在第一次BBF事件中,空间观测和地面观测均发现了Pi2脉动;在第二次事件中,地面观测到了Pi2脉动,而空间没有观测到Pi2脉动;在第三次事件中,空间和地面观测都没有发现Pi2脉动.这些观测事实说明BBF所激发的Pi2脉动特征是相当复杂的,而且并不是所有BBF都能产生Pi2脉动,所以到底BBF在什么条件下可以产生Pi2仍然是一个没有解决的问题.   相似文献   

16.
Solar particle events can give greatly enhanced radiation at aircraft altitudes, but are both difficult to predict and to calculate retrospectively. This enhanced radiation can give significant dose to aircrew and greatly increase the rate of single event effects in avionics. Validation of calculations is required but only very few events have been measured in flight. The CREAM detector on Concorde detected the event of 29 September 1989 and also four periods of enhancement during the events of 19-24 October 1989. Instantaneous rates were enhanced by up to a factor ten compared with quiet-time cosmic rays, while flight-averages were enhanced by up to a factor six. Calculations are described for increases in radiation at aircraft altitudes using solar particle spectra in conjunction with Monte Carlo radiation transport codes. In order to obtain solar particle spectra with sufficient accuracy over the required energy range it is necessary to combine space data with measurements from a wide range of geomagnetically dispersed, ground-level neutron monitors. Such spectra have been obtained for 29 September 1989 and 24 October 1989 and these are used to calculate enhancements that are compared with the data from CREAM on Concorde. The effect of cut-off rigidity suppression by geomagnetic activity is shown to be significant. For the largest event on record on 23 February 1956, there are no space data but there are data from a number of ground-level cosmic-ray detectors. Predictions for all events show very steep dependencies on both latitude and altitude. At high latitude and altitude (17 km) calculated increases with respect to cosmic rays are a factor 70 and 500 respectively for 29 September 1989 and 23 February 1956. The levels of radiation for high latitude, subsonic routes are calculated, using London to Los Angeles as an example, and can exceed 1 mSv, which is significantly higher than for Concorde routes from Europe to New York. The sensitivity of the calculations to spectral fitting, geomagnetic activity and other assumptions demonstrates the requirement for widespread carriage of radiation monitors on aircraft.  相似文献   

17.
In this paper, the estimation capacities of MLR and ANN are investigated to estimate monthly-average daily SR over Turkey. The satellite data are used for 73 different locations over Turkey. Land surface temperature, altitude, latitude, longitude and month are offered as the input variables for modeling ANN and MLR to get SR. Estimations of SR are evaluated with the meteorological values by using the statistical bases. The obtained results indicated that the ANN model could achieve a satisfactory performance when compared to the MLR model. Moreover, it is understood that more accurate results in estimation of SR are obtained in the use of satellite data, rather than the use of meteorological station data. Finally, the built ANN model is used to estimate the yearly average of daily SR over Turkey. As a result, satellite-based SR map for Turkey is generated.  相似文献   

18.
基于子午工程北大深圳站(22.59°N,113.97°E)电离层GPS双频接收机在2011年1月1日至2017年12月31日连续7年的长时间序列闪烁和TEC观测数据,分析不同太阳活条件下华南赤道异常北驼峰区观测到的GPS卫星L波段电离层闪烁事件时空分布特征及其对通信的影响.结果表明:GPS闪烁事件几乎都发生在夜间,且主要发生在春秋分月份;在不同太阳活动条件下,夜间GPS闪烁事件都主要发生在北驼峰区域靠近磁赤道的一侧,且GPS闪烁事件存在明显的东-西侧天区不对称性,即在台站西侧天区发生的闪烁事件明显偏多;在不同太阳活动条件下,弱闪烁事件伴随的TEC耗尽和卫星失锁事件比例相对较低,强闪烁事件则大部分都伴随着TEC耗尽和卫星失锁事件的发生.   相似文献   

19.
On 14 October 1999, the Chinese-Brazil earth resource satellite (CBERS-1) was launched in China. On board of the satellite there was an instrument designed at Peking University to detect the energetic particle radiation inside the satellite so the radiation fluxes of energetic particles in the cabin can be monitored continuously. Inside a satellite cabin, radiation environment consists of ether penetrated energetic particles or secondary radiation from satellite materials due to the interactions with primary cosmic rays.Purpose of the detectors are twofold, to monitor the particle radiation in the cabin and also to study the space radiation environment The data can be used to study the radiation environment and their effects on the electronics inside the satelhte cabin. On the other hand, the data are useful in study of geo-space energetic particle events such as solar proton events, particle precipitation and variations of the radiation belt since there should be some correlation between the radiation situation inside and outside the satellite.The instrument consists of two semi-conductor detectors for protons and electrons respectively. Each detector has two channels of energy ranges. They are 0.5-2MeV and ≥2MeV for electrons and 5-30MeV and 30-60MeV for protons. Counting rate for all channels are up to 104/(cm2@s)and power consumption is about 2.5 W. There are also the additional functions of CMOS TID (total integrated dose) effect and direct SEU monitoring. The data of CBMC was first sent back on Oct. 17 1999 and it's almost three years from then on. The detector has been working normally and the quality of data is good.The preliminary results of data analysis of CBMC not only reveal the effects of polar particle precipitation and radiation belt on radiation environment inside a satellite, but also show some important features of the geo-space energetic particle radiation.As one of the most important parameters of space weather, the energetic charged particles have great influences on space activities and ground tech nology. CBMC is perhaps the first long-term on-board special equipment to monitor the energetic particle radiation environment inside the satellite and the data it accnmulated are very useful in both satellite designing and space research.  相似文献   

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