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GPS和GLONASS卫星定位系统分别采用WGS-84和PZ-90坐标系。为统一两种卫星定位成果,欧、美、俄于20世纪90年代各自求出两坐标系之间的转换参数。目前三种参数尚未统一,对GPS/GLONASS联合定位造成较大影响。本文针对国外介绍PZ-90和WGS-84坐标系相互转换时常用的转换模型及三种不同转换参数进行比较分析。分别选用地面GPS参考站坐标和GLONASS卫星轨道坐标,用三种坐标转换参数进行转换,对转换结果差异及其对单点定位和相对定位精度造成的影响进行全面分析比较,得出一些有益结论。 相似文献
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王解先 《大地测量与地球动力学》2007,27(2):43-46
?????????????????????WGS84?????????????????????????????????????????????????????????????????????????????????????????????????????????????С??Χ???????????????????????????????????????????????????????????Ч??? 相似文献
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����ο���ܵ�ʵ�ֺ�ά�� 总被引:1,自引:2,他引:1
??ITRF??WGS84??ο?????????????ο???????????????????????????????????Щ?????????????? ????????,??????°汾ITRF2005?????????? 相似文献
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��ά�ռ����ά�ռ��߲���ת����������·��� 总被引:6,自引:1,他引:5
????????????δ?????????????????????????????????·?????????????????????????????????????????????????????????÷?Χ???ó?????:????γ??????Χ??С??8???,??x??y???????????????1 cm??????????侫???????γ??(?????γ??)??Χ????С?????????? 相似文献
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Witold Maciejewski James Binney 《Monthly notices of the Royal Astronomical Society》2001,323(4):831-838
We consider long-slit emission-line spectra of galactic nuclei when the slit is wider than the instrumental point spread function, and the target has large velocity gradients. The finite width of the slit generates complex distributions of brightness at a given spatial point in the measured spectrum, which can be misinterpreted as coming from additional physically distinct nuclear components. We illustrate this phenomenon for the case of a thin disc in circular motion around a nuclear black hole (BH). We develop a new method for estimating the mass of the BH that exploits a feature in the spectrum at the outer edge of the BH's sphere of influence, and therefore gives higher sensitivity to BH detection than traditional methods. Moreover, with this method we can determine the BH mass and the inclination of the surrounding disc separately, whereas the traditional approach to BH estimation requires two long-slit spectra to be taken. We show that, with a given spectrograph, the detectability of a BH depends on the sense of rotation of the nuclear disc. We apply our method to estimate the BH mass in M84 from a publicly available spectrum, and recover a value four times lower than that published previously from the same data. 相似文献
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针对WGS-84CGCS2000坐标基准差异问题,分析了用于估计基准转换参数的Bursa模型及其求解方法,初步尝试求取WGS-84CGCS2000的坐标基准转换参数。算例采用了中国区域内含有CGCS2000坐标值,同时安装有GPS接收机的21个观测站,并针对点位的区域分布问题,提出利用重心化的Bursa模型求解转换参数的思路,且得到一组较好的转换结果。 相似文献
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一种快速获取GPS控制网精确WGS-84坐标方法 总被引:1,自引:0,他引:1
详细介绍了一种快速求取GPS控制网的精确WGS-84坐标的方法。首先选择三个天空通视条件较好、分布合理的控制网点,与附近的IGS跟踪站进行长基线相对定位或者直接进行静态精密单点定位,求得三点精确的WGS-84坐标,然后将这三个点作为已知点在WGS-84坐标系下进行三维约束平差,可求得控制网其它点精确的WGS-84坐标,这样求得网点的WGS-84坐标具有厘米级精度。 相似文献
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3C 84 is a well-known supermassive black hole that can be used to explore jet and accretion physics. In this work, we model the multiwavelength spectral energy distribution (SED) of the 3C 84, and find that the SED is difficult to fit with pure advection dominated accretion flow (ADAF) or pure jet model. Using a coupled ADAF-jet model to fit the SED of 3C 84, it is found that the radio emission and the millimeter emission can be naturally reproduced by the synchrotron radiation of nonthermal electrons in the jet, and that the X-ray emission may predominantly come from inverse Compton radiation from electrons in ADAF. According to the Rotation Measure (RM) obtained by the polarization observation, we consider the possible location of the polarizing source and found that the calculated RM in the jet is roughly consistent with the observational constraints. These results will help us better understand jets produced by black holes. 相似文献