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181.
F—P腔作为光滤波器用.具有稳定性高.通带窄的优点。采用低精细度的法布里-珀罗滤波器(F—P)直接提出帧时钟,保证时钟的快速建立和快速消失。利用半导体光放大器(SOA)的自增益调制效应(SGM)对F-P提取的帧时钟进行整形,降低帧时钟的幅度噪声。并推导了F—P的精细度Q和SOA的自增益调制效应对帧时钟建立时间、消失时间的影响。通过理论分析表明,利用SOA的SGM效应可以降低帧时钟的幅度噪声并加快帧时钟建立速度。实验中,用上述方案对10.075GHz的帧信号进行了全光帧时钟提取.得到了建立时间为8个信号周期.消失时间为22个信号周期抖动为2.35ps的帧时钟信号. 相似文献
182.
Guiping Liu Gordon G. Shepherd 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The yearly variation of the integrated emission rate of the O(1S) nightglow in the lower thermosphere is studied and the solar cycle impact is examined from the observations of the Wind Imaging Interferometer (WINDII) operated on the Upper Atmosphere Research Satellite (UARS). More than 300,000 volume emission rate profiles of the O(1S) nightglow observed by WINDII for 40°S–40°N latitudes during November 1991–August 1997 over half of a solar cycle are utilized. These profiles are vertically integrated for the altitude range of 80–100 km and the equivalent column integrated emission rates are then zonally averaged for bins with 10° latitude and 3 month intervals. It is found that for each latitude the O(1S) nightglow emission rate appears to increase with increasing solar F10.7 cm flux, following a linear relationship. This characterizes the solar cycle impact on the O(1S) nightglow, while the solar influence is modulated by a seasonal variation. Based on these variations, an empirical formula is derived for predicting the three-month averages of the O(1S) nightglow integrated emission rate. The standard error of the estimated values from the formula is smaller than 30 Rayleigh. 相似文献
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184.
磁选态铯原子钟的输出频率与铯束管输出的弱电流信号有关,影响其频率稳定度。为了提高其频率稳定度技术指标,在对磁选态铯原子钟主伺服电路弱信号压频转换(V-F)和模/数 (A/D)直接采样对比的基础上,设计了基于DSP28335芯片的A/D直接采样电路,利用CAN总线通信技术与主控CPU板进行通信,实现整钟闭环锁定的方案。通过试验与被测磁选态铯原子钟现有压频转换法进行对比,结果表明,所设计的A/D直接采样法较压频转换法减小了磁选态铯原子钟相对频率偏差范围,改善了短期频率稳定度,具有实用价值。 相似文献
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186.
A new stochastic model considering satellite clock interpolation errors in precise point positioning
Shengli Wang Fanlin Yang Wang Gao Lizi Yan Yulong Ge 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(5):1332-1341
Precise clock products are typically interpolated based on the sampling interval of the observational data when they are used for in precise point positioning. However, due to the occurrence of white noise in atomic clocks, a residual component of such noise will inevitable reside within the observations when clock errors are interpolated, and such noise will affect the resolution of the positioning results. In this paper, which is based on a twenty-one-week analysis of the atomic clock noise characteristics of numerous satellites, a new stochastic observation model that considers satellite clock interpolation errors is proposed. First, the systematic error of each satellite in the IGR clock product was extracted using a wavelet de-noising method to obtain the empirical characteristics of atomic clock noise within each clock product. Then, based on those empirical characteristics, a stochastic observation model was structured that considered the satellite clock interpolation errors. Subsequently, the IGR and IGS clock products at different time intervals were used for experimental validation. A verification using 179 stations worldwide from the IGS showed that, compared with the conventional model, the convergence times using the stochastic model proposed in this study were respectively shortened by 4.8% and 4.0% when the IGR and IGS 300-s-interval clock products were used and by 19.1% and 19.4% when the 900-s-interval clock products were used. Furthermore, the disturbances during the initial phase of the calculation were also effectively improved. 相似文献
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188.
针对卫星钟差序列中非线性特性较为复杂和超快速钟差预报精度较低的问题,将核极限学习机算法引入到北斗超快速钟差预报中。首先,将极限学习机进行优化,引入粒子群优化算法来选择核极限学习机所需的核参数和正则化参数;然后,将优化后的方法应用到超快速钟差预报中,并给出了利用该方法进行超快速钟差预报的步骤;最后,在分析iGMAS提供的实测北斗超快速钟差数据的基础上,选用单天和多天数据进行短期预报。结果表明:在短期预报6h范围内,利用本文提供的优化方法解算得到的超快速钟差预报精度明显优于二次多项式模型和周期项模型,并且采用此方法得到的超快速钟差预报产品与iGMAS提供的超快速钟差预报产品(ISU-P)相比,GEO、IGSO和MEO卫星的预报精度分别提升了50.51%、46.98%、40.67%,其与最终精密钟差的符合程度显著 增强 。 相似文献
189.
Nabil Ben Nessib Norah Alonizan Rabia Qindeel Sylvie Sahal-Bréchot Milan S. Dimitrijević 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Line ratio of O IV 1407.3 Å/1401.1 Å is calculated using mostly our own atomic and collisional data. 相似文献
190.