期刊文献+

基于Hermite展开的太阳闪烁时间序列产生器

Solar Scintillation Time Series Generation Based on Hermite Expansion
下载PDF
导出
摘要 研究太阳闪烁产生器设计优化问题,由于受太阳活动的影响,深空通信十分复杂。在无线通信中常受到太阳闪烁的影响,产生误码,造成通信效率降低。为了测试深空通信设备性能,一定要了解太阳闪烁时间序列的性能特点。针对实际观测得到的太阳闪烁时间序列极少的问题,在分析太阳闪烁特性的基础上,提出了一种用Hermite展开的太阳闪烁时间序列产生方法,并与基于FIR滤波器的闪烁时间序列产生方法进行了比较。仿真结果表明,提出的基于Hermite展开的太阳闪烁时间序列产生的性能,优于基于FIR滤波器的闪烁时间序列产生方法,并且无需预先知道时间序列的概率分布特性,更具有实用性,为太阳闪烁产生器设计提供了依据。 Research for the optimization problem of the solar scintillation time series generation's design.Due to the influence of the sun's activity,deep space communication is very complicated.In the wireless communication,due to the influence of the solar scintillation,it produces error and causes low efficiency.In order to test the performance of the deep space communication equipment,we must understand the characteristics of the solar scintillation time series.Because the solar scintillation time series of the actual observation is very little,based on the analysis of the characteristics of the solar scintillation,this paper researched a solar scintillation time series generation based on Hermite expansion,and compared with the solar scintillation time series generation based on FIR filter.The simulation results show that the performance of the solar scintillation time series generation based on Hermite expansion is better than the solar scintillation time series generation based on FIR filter,and this generation does not need to determine the probability distribution characteristics of the solar scintillation time series,so it is more practical.
出处 《计算机仿真》 CSCD 北大核心 2012年第10期400-404,共5页 Computer Simulation
基金 贵州省省长基金项目(2008(28))
关键词 太阳闪烁 信号功率谱 埃尔米特展开式 时间序列 Solar scintillation Signal power spectrum Hermite expansion Time series
  • 相关文献

参考文献14

  • 1胡圣波,孟新,赵娜,蒋立正.弱太阳闪烁中的深空探测信道预测[J].宇航学报,2009,30(1):244-249. 被引量:6
  • 2赵娜,孟新,胡圣波.弱太阳闪烁对深空通信的影响[J].空间科学学报,2009,29(2):244-248. 被引量:10
  • 3Y Beniguel, J P Adam. Time series generators to simulate earth satellite links affected by scintillations[ C]. Antennas and Propaga- tion, Nov 11 -16, 2007:1 -4.
  • 4J Sala, M Lamarca. A Rain and Scintillation Ka - band Channel Simulator[ C ]. Signal Processing for Space Communications, Oct 6 -8, 2008:1 -4.
  • 5Lisha Sun, Minfen shen. Model for generation non - Gaussian noise sequences having specified probability distribution and spec- trum[J]. Parallel and Distributed Computing: Applications and Technologies Lecture Notes in Computer Science, 2005, Volume 3320/2005:157 - 183.
  • 6M Shen, F H Y Chan. A method for generating non - Gaussian noise series with specified probability distribution and power spec- trum[ C]. IEEE Internation Symposium on Circuits and Systems Proceedings, Bangkok, Thailand, May 25 - 28 2003,2 : 1 - 4.
  • 7Liu Bede, D Jr Munson. Generation of a random sequence having a jointly specified marginal distribution and auto - covariance [ C ]. Acoustics, Speech, and Signal Processing, IEEE Transactions on, Dec 1982,30(6) :973 -983.
  • 8D Morabito. Solar Corona Amplitude Scintillation Modeling and Comparison to Measurements at X - Band and Ka - Band[ R]. The Telecommunications and Data Acquisition Progress Report 42 - 153, JPL Pasadena, California, May 15, 2003.
  • 9R Woo. Measurements of the solar wind using spacecraft radio scat- tering observations [ M ]. In: Study of Traveling Interplanetary Phe- nomena, Dordrecht - Holland, The Netherlands: D Reidel, 1977 : 81 - 100.
  • 10叶品中,邱育海.行星际闪烁(IPS)单站观测对太阳风速度的诊断[J].天体物理学报,1996,16(4):389-394. 被引量:8

二级参考文献24

  • 1刘嘉兴.深空测控通信的特点和主要技术问题[J].飞行器测控学报,2005,24(6):1-8. 被引量:23
  • 2叶品中,邱育海.行星际闪烁(IPS)单站观测对太阳风速度的诊断[J].天体物理学报,1996,16(4):389-394. 被引量:8
  • 3叶品中.行星际闪烁功率谱的Fresnel现象与太阳风速度[J].空间科学学报,1996,16(3):172-177. 被引量:4
  • 4David Morabito, Roll Hastrup. Communicating with mars during periods of solar conjunction[C]//Proceedings of IEEE Aerospace Conference, 2002, Big Sky, Montana, March 9- 16,2002:1271 - 1281.
  • 5Eyceoz T, Duel-Hallen A, Hallen H. Prediction of fast fading Parameters by resolving the interference pattern[ C]//Proceedings of the 31st ASILOMAR Conference on Signals, Systems, and Computers. Pacific Grove, CA,1997: 167- 171.
  • 6Ekman T, Kubin G. Nonlinear prediction of mobile radio channels M easurements and MARS model designs[ C]//Proceedings of Int. Conf. Accust. Speech Sig. Process. Phoenix, A Z,March 1999: 2667- 2670.
  • 7Davis D, Morabito. The Cassini May 2000 Solar Conjunction. IEEE Trans. on Antennas and Propagation, 2003, 51 (2) : 201 - 219.
  • 8Morabito D. Solar Corona Amplitude Scintillation Modeling and Comparison to Measurements at X-Band and Ka-Band[ R]. The Telecommunications and Data Acquisition Progress Report 42 - 153, JPL Pasadena, California, May 15,2003.
  • 9Woo R. Measurements of the solar wind ug spacecraft radio scattering observations. Study of Traveling Interplanetary Phenomena, Dordrecht-HoUand, The Netherlands : D. Reidel, 1977 : 81 - 100.
  • 10Feria Y, Belongie M, McPheeters T, Tan H. Solar Scintillation Effects on Communication Links at Ka-band and X-band[ RI. The Teleand Data Acquisition Progress Report 42 - 129, JPL Pasadena, California, May 15, 1997

共引文献16

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部