GPS中BOC调制的FPGA实现     

刘音华  卢晓春  边玉敬 《时间频率学报》2006,29(1):35-42

GPS系统中提出了一种新的信号形式,二进制偏移载波(BOC)调制是这种新的信号形式产生的技术关键。首先介绍了BOC调制的定义及其频谱特性,然后阐述了基于FPGA(现场可编程门阵列)硬件平台的BOC调制实现方法,并给出了仿真波形。结果表明,该实现方法是值得提倡的。  相似文献   

雷达回波二进制源文件转换成透明GIF图像文件的方法     

史彩霞  刘世学 《气象研究与应用》2002,23(Z1):54-55

详细介绍了雷达回波二进制源文件转换成透明GIF图像文件的方法.  相似文献   

可视化修改二进制数据文件   总被引：1，自引：0，他引：1  

李玉红  吴坤椿 《广西气象》2002,23(3):50-51

利用Visual Basic语言，TEXTBOX控件的特性，全屏幕修改二进制数据文件。  相似文献   

利用二进制特征描述符的改进SIFT影像匹配算法     

于翔舟  王慧  李烁  杨乐  闸旋 《海洋测绘》2019,39(1):39-43

针对SIFT算法在匹配过程中运行效率低的不足,结合BRIEF特征描述子,将SIFT算法的高维特征向量转换为二进制特征描述子,以提高匹配效率。特征匹配过程首先采用Hamming距离完成粗匹配,再采用最小距离筛选法结合PROSAC算法的双重检测对初步匹配的特征点去伪,获得精准的匹配点对。实验结果表明该算法较SIFT算法匹配精度平均提升30.6%,匹配效率平均提高4.06倍,具有较强的实时性以及可行性。  相似文献   

基于SQL Server数据库的遥感影像数据存储的策略与方法     

郑浩张蔚  刘继东 《测绘技术装备》2006,8(1):22-24

对遥感影像数据进行高效、快捷地存储与管理,已经成为一种迫切需求。本文讲述了如何使用SQLSERVER数据库存储遥感影像数据的策略与方法。  相似文献   

BOC调制信号多径误差分析     

赵薇薇  李春霞 《测绘学院学报》2009,(4)

针对导航信号的多径误差分析,在多径误差包络曲线分析方法基础上提出了多径误差包络期望分析方法。与包络曲线分析方法相比,包络期望分析方法能够定量分析导航信号多径误差。基于包络期望分析方法,对同码速率的二进制偏移载波(BOC)调制导航信号与二进制相位控键(BPSK)调制导航信号的多径误差进行了对比分析。结果表明,BOC调制导航信号具有更小的典型多径误差。  相似文献   

ArcGIS8图形二进制解读     

高铁军  赵丹  佟大辉 《测绘科学》2006,31(3):85-88

通过对ArcG IS8 Personal Geodatabase和Enterprise Geodatabase图形二进制字段存储规律的解读,完成脱离ArcG IS环境,使用ADO直接对ArcG IS地理数据库图形二进制字段进行读写操作,为地理资源共享提供了一种新途经,同时提高了ArcG IS8地理数据库应用的灵活性。  相似文献   

BOC调制信号抗干扰能力分析     

李春霞  楚恒林  王宏兵 《测绘科学技术学报》2012,(6):414-417

抗干扰能力是卫星导航信号设计的一项重要考核要素。目前典型的方法是采用抗干扰品质因数、伪码跟踪精度下降来衡量。但是该抗干扰品质因数不能反映码速率对抗干扰能力的贡献,而伪码跟踪精度下降则不够简捷。提出了能够反映伪码速率贡献的载波跟踪抗干扰品质因数,以及能够简捷地反映伪码跟踪抗干扰能力的伪码跟踪抗干扰品质因数。采用所提出的两项指标,对二进制偏移副载波BOC(Binary Offset Carrier)调制这一新型卫星导航信号进行了抗干扰能力分析。结果表明,同码率BOC调制信号载波跟踪抗干扰能力比BPSK调制信号强,伪码跟踪抗干扰能力比BPSK调制信号弱。  相似文献   

An orbital period investigation of the Algol-type eclipsing binary VW Hydrae     

Jia Zhang Sheng-Bang Qian Boonrucksar Soonthomthum 《中国天文和天体物理学报》2009,9(3)

Orbital period variations of the Algol-type eclipsing binary, VW Hydrae, are analyzed based on one newly determined eclipse time and the other times of light minima collected from the literature. It is discovered that the orbital period shows a continuous increase at a rate of dP/dt = +6.34×10-7 d yr-1 while it undergoes a cyclic change with an amplitude of 0.0639 d and a period of 51.5 yr. After the long-term period increase and the large-amphtude period oscillation were subtracted from the O-C curve, the residuals of the photoelectric and CCD data indicate a small-amplitude cyclic variation with a period of 8.75 yr and a small amplitude of 0.0048d. The continuous period increase indicates a conservative mass transfer at a rate of dM2/dt = 7.89×10-8 M⊙ yr-1 from the secondary to the primary. The period increase may be caused by a combination of the mass transfer from the secondary to the primary and the angular momentum transfer from the binary system to the circumbinary disk. The two cyclic period oscillations can be explained by light-travel time effects via the presence of additional bodies. The small-amplitude periodic change indicates the existence of a less massive component with mass M3 > 0.53 M⊙, while the large-amplitude one is caused by the presence of a more massive component with mass M4 > 2.84 M⊙. The ultraviolet source in the system reported by Kviz & Rufener (1987) may be one of the additional components, and it is possible that the more massive one may be an unseen neutron star or black hole. The rapid period increase and the possibility of the presence of two additional components in the binary make it a very interesting system to study. New photometric and high-resolution spectroscopic observations and a detailed investigation of those data are required in the future.  相似文献   

An unusual timing and spectral state of a black hole microquasar XTE J1550-564     

Ying-Kang Jin Shuang-Nan Zhang Ti-Pei Li 《中国天文和天体物理学报》2009,9(2)

An unusual timing and spectral state of a black hole microquasar XTE J1550-564 observed with RXTE is analyzed. Millisecond variabilities are found, which are significantly shorter than the minimum possible time scale in the light curves of black hole binaries, as suggested by Sunyaev & Revnivtsev (2000). The X-ray spectral fitting result indicates that there is an unusual soft component in the spectrum, which may be responsible for the millisecond variabilities. The millisecond variabilities as well as the unusual soft spectral component should be produced from some small, but independent active regions in the accretion disk.  相似文献