物理学报
物理學報
물이학보
2013年
10期
510-520
,共11页
孙海峰%谢楷%李小平?%方海燕%刘秀平%傅灵忠%孙海建%薛梦凡
孫海峰%謝楷%李小平?%方海燕%劉秀平%傅靈忠%孫海建%薛夢凡
손해봉%사해%리소평?%방해연%류수평%부령충%손해건%설몽범
X射线光子信号%时间稳定度%观测脉冲轮廓%导航算法
X射線光子信號%時間穩定度%觀測脈遲輪廓%導航算法
X사선광자신호%시간은정도%관측맥충륜곽%도항산법
X-ray pulsar signal%timing stability%observation profile%navigation algorithms
X射线脉冲星导航是一种完全自主的导航方式,在深空乃至行星际空间具有潜在的工程应用价值.由于空间飞行试验系统复杂,成本巨大,在实验室环境下高精度地模拟X射线脉冲星信号对数据处理方法和导航方案的验证具有重要意义.针对当前机械转盘式模拟系统中时间稳定度和轮廓精度的不足,提出了一种通过产生的轮廓电压信号直接控制可见光光源,再利用衰减获得光子流,最后经单光子探测和处理电路输出光子到达时间序列的模拟新方法.该方法实现成本低,支持任意X射线脉冲星信号的模拟,且具有高时间稳定度和轮廓精度.详细地讨论了该方法的原理和涉及的关键技术,搭建了X射线脉冲星信号模拟系统,并进行了实验.实验结果表明:该系统大幅提高了X射线脉冲星信号的模拟效果,将模拟脉冲星自转周期的稳定度从现有的10?4提高到10?9;当探测器面积为1 m2,探测能谱范围为2—10 keV,积分时间为1200 s时,模拟的PSR B1509?58观测脉冲轮廓与标准脉冲轮廓的相关系数达到了0.993.
X射線脈遲星導航是一種完全自主的導航方式,在深空迺至行星際空間具有潛在的工程應用價值.由于空間飛行試驗繫統複雜,成本巨大,在實驗室環境下高精度地模擬X射線脈遲星信號對數據處理方法和導航方案的驗證具有重要意義.針對噹前機械轉盤式模擬繫統中時間穩定度和輪廓精度的不足,提齣瞭一種通過產生的輪廓電壓信號直接控製可見光光源,再利用衰減穫得光子流,最後經單光子探測和處理電路輸齣光子到達時間序列的模擬新方法.該方法實現成本低,支持任意X射線脈遲星信號的模擬,且具有高時間穩定度和輪廓精度.詳細地討論瞭該方法的原理和涉及的關鍵技術,搭建瞭X射線脈遲星信號模擬繫統,併進行瞭實驗.實驗結果錶明:該繫統大幅提高瞭X射線脈遲星信號的模擬效果,將模擬脈遲星自轉週期的穩定度從現有的10?4提高到10?9;噹探測器麵積為1 m2,探測能譜範圍為2—10 keV,積分時間為1200 s時,模擬的PSR B1509?58觀測脈遲輪廓與標準脈遲輪廓的相關繫數達到瞭0.993.
X사선맥충성도항시일충완전자주적도항방식,재심공내지행성제공간구유잠재적공정응용개치.유우공간비행시험계통복잡,성본거대,재실험실배경하고정도지모의X사선맥충성신호대수거처리방법화도항방안적험증구유중요의의.침대당전궤계전반식모의계통중시간은정도화륜곽정도적불족,제출료일충통과산생적륜곽전압신호직접공제가견광광원,재이용쇠감획득광자류,최후경단광자탐측화처리전로수출광자도체시간서렬적모의신방법.해방법실현성본저,지지임의X사선맥충성신호적모의,차구유고시간은정도화륜곽정도.상세지토론료해방법적원리화섭급적관건기술,탑건료X사선맥충성신호모의계통,병진행료실험.실험결과표명:해계통대폭제고료X사선맥충성신호적모의효과,장모의맥충성자전주기적은정도종현유적10?4제고도10?9;당탐측기면적위1 m2,탐측능보범위위2—10 keV,적분시간위1200 s시,모의적PSR B1509?58관측맥충륜곽여표준맥충륜곽적상관계수체도료0.993.
@@@@A simulation experiment system is required presently, for the space flight experiment of X-ray pulsar based navigation is very costly. To solve the crucial issues of the timing stability and the profile precision in existing simulation techniques of pulsar signal, a new simulation technique which utilizes visible light is proposed. The simulation experiment system is set up based on the proposed technique. And some experiments are carried out to test the proposed technique. The results demonstrate that the proposed technique can be used to simulate any of known pulsars. The timing stability of simulated X-ray pulsars is raised from 10?4 to 10?9. And the accuracy of pulsar profile simulation is noticeably improved. Within the X-ray band 1–10 keV, when the observation time reaches 1200 s, and the area of the X-ray detector is 1 m2, the Pearson correlation coefficient of pulsar’s observation profile with the standard template profile arrives at 0.993. And the simulation experiment system can be realized with high flexibility and low cost. On the basis of the simulation experiment system, the signal characteristic of X-ray pulsar can be investigated. On the other hand, the performances of X-ray pulsar signal processing algorithms and navigation algorithms can be surveyed in detail.