开源软件定制改造过程中的原型选择

在定制改造开发过程中选择合适的原型系统,可以达到提高定制改造过程效率、减少开发成本、缩短开发周期的目的.在定制改造过程的原型分析和评估中依托构造成本模型COCOMO(COstructive COst MOdel) II,提出一种新的软件成本评估方法,综合分析了影响定制改造过程的功能差异、性能、规模、稳定性等关键因素,量化了这些关键因素对定制改造过程中成本计算公式中的关键变量——等价代码——的影响.实际的项目显示,该方法对预期工作量的估计误差约为17%,远小于COCOMO II模型40%的可接受阈值.      

FSK副载波光纤传输的灵敏度分析

在光纤传输系统中，副载波光纤传输是一种独特的传输方式，以ＭＩＬ－ＳＴＤ－１７７３年推荐的ＦＳＫ副载波光纤传输为例，对光接收机噪声及误率进行了分析，提出在色噪声情况下常规接收机的判决门限修正，为了简化计算起见，给出一种近似计算的方法，经计算，得到了副载波ＦＳＫ在不同接收机组态及码速率情况下的灵敏度曲线，并与常见的曼彻斯特码作了对比，分析了副载波光纤传输在不同场合时的性能。     

A genetic algorithm for Initial Orbit Determination from a too short arc optical observation

Optical observations constitute a source of angular measurements of a satellite pass. Commonly, these observations have short durations with respect to the satellite orbit period. As a consequence, the use of classical orbit determination algorithms, as Laplace, Gauss or Escobal methods, give very poor results. The present work faces with the problem of estimating the orbital parameters of an orbiting object using its optical streak acquired by a telescope or a high accuracy camera. In the paper a new technique is developed for the Initial Orbit Determination from optical data by exploiting the genetic algorithms. The algorithm works without restrictions on the observer location. A recent challenging problem is the Initial Orbit Determination with space-based observations. This work focuses on the problem of determinating the orbital parameters of a satellite from an orbiting observer in LEO, using short time observations. We present the results based on a simulation with the observer on a sun-synchronous orbit with a single observation of just 60 s. Monte Carlo simulations are presented with different levels of sensor accuracy to show the reliability of the algorithm. The algorithm is able to yield a candidate solution for each observation. The coplanar case is analyzed and discussed as well.     

全定制芯片的测试码产生方法

针对全定制设计的芯片提出人工产生测试码的方法.该方法充分利用功能验证程序,从中挑选出对测试有用的信息,经过转换得到满足基本故障覆盖的测试码;再结合芯片自身的结构特点,合理利用芯片内部的调试结构,并按功能部件利用调试链路追加测试码,从而补充完善得到比较完备的测试码.     

混沌码用作测控扩频码的可行性研究

阐述了混沌码的基本特性,提出用混沌码作为测控扩频码的构想,并讨论了混沌码扩频测控体系构成,以及体系中的关键技术,从而论证混沌码扩频测控体制的可行性,研究表明混沌码比传统扩频码有更强的保密和抗多址干扰特性。     

一种基于MATLAB快速开发跨平台算法软件的方法

利用MATLAB进行算法的研究、仿真和实现，已经成为科研工作者的重要手段之一。在MATLAB上开发算法便捷、高效，但无法直接应用在其他平台，此时需要软件人员编码转换进行二次开发。如果某个算法同时应用在Windows和Linux这两个系统中，软件人员需要开发两个不同的软件，它们功能相同只是代码不同。这不仅增加了软件开发的工作量，同时也不利于后期维护。针对上述问题，提出了一种基于MATLAB快速开发跨平台算法软件的方法。首先，利用MATLAB开发算法的便捷性进行算法的调试与验证，简化接口函数；其次，使用MATLAB Coder生成独立于MATLAB的C/C++代码；然后，将生成的代码在不同平台下进行封装，生成该目标平台的动态链接库；最后，不同平台通过调用该平台下的动态链接库，实现了同一算法的跨平台软件开发。所提出的算法软件跨平台开发方法，已成功应用于多个实际项目。通过本方法，不仅缩短了软件的开发周期，提高了软件编程效率，减少了软件开发中的人为错误，同时方便了软件的后期维护。     

Grouping bi-chi-squared method for pulsar navigation experiment using observations of Rossi X-ray timing explorer

X-ray pulsar-based navigation is a revolutionary technology which is capable of providing the required navigation information in the solar system. Performing as an important pulsar-based navigation technique, the Significance Enhancement of Pulse-profile with Orbit-dynamics (SEPO) can estimate orbital elements by using the distortion of pulse profile. Based on the SEPO technique, we propose a grouping bi-chi-squared technique and adopt the observations of Rossi X-ray Timing Explorer (RXTE) to carry out experimental verification. The pulsar timing is refined to determine spin parameters of the Crab pulsar (PSR B0531+21) during the observation periods, and a short-term dynamic model for RXTE satellite is established by considering the effects of diverse perturbations. Experimental results suggest that the position and velocity errors are 16.3 km (3σ) and 13.3 m/s (3σ) with two adjacent observations split by one day (exposure time of 1.5 ks), outperforming those of the POLAR experiment whose results are 19.2 km (3σ) and 432 m/s (3σ). The approach provided is particularly applicable to the estimation of orbital elements via using high-flux observations.     

The potential of Meudon spectroheliograph for investigating long term solar activity and variability

Observations of the chromosphere with Deslandres’s spectroheliograph started at Paris Observatory in 1893 and were followed by systematic observations at Meudon since 1908. The solar collection of H$\alpha$ and CaII K images is probably the longest available worldwide, with associated products such as synoptic maps and tables. Since 2018, Meudon spectroheliograph is the only instrument producing data-cubes of full line profiles of CaII H, CaII K and H$\alpha$, for each pixel of the solar disk. Slices of the cubes provide monochromatic images. We summarize in this paper the capabilities of the successive generations of the instrument, and explore the potential of the collection and products for analysis of rare events, investigations of past solar activity and studies of long term variability.     

Blind identification of space–time block codes based on deep learning

Deep Learning(DL) has important applications to both commercial and military communications, such as software-defined radio, cognitive radio and spectrum surveillance. While DL has been intensively studied for modulation recognition, there are very few investigations for blind identification of Space-Time Block Codes(STBCs). This paper proposes a Residual Network(RN)-based model for identifying 6 kinds of STBC signals with a single receiving antenna, including the same length of coding matrix. I...     

城市环境下北斗B-CNAV1电文RS-LDPC 级联编码方法

针对城市环境下卫星导航系统用户接收终端对电文编译码算法的低复杂度和抗衰落性能需求，以北斗导航系统B-CNAV1电文为改进对象提出了一种外码采用RS码、内码采用二进制LDPC码的电文级联编码方法。通过RS码提高电文对抗突发错误的能力，同时利用二进制LDPC码保证电文对抗随机错误的能力。采用LMS信道对城市接收环境建模，仿真结果验证了本文提出的RS-LDPC级联码与B-CNAV1电文64进制LDPC码具有相近的性能，同时大幅降低了算法复杂度，较好地实现了电文纠错性能和实现复杂度的平衡，提供了一种适用于城市环境的高性能、低复杂度电文编码方法。