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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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�߲���ת���в���֮�������� 总被引:8,自引:7,他引:8
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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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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2000国家大地坐标系椭球参数与GRS 80和WGS 84的比较 总被引:15,自引:2,他引:13
根据2000国家大地坐标系(CGCS 2000)的定义及其所定义的4个基本椭球常数,推导CGCS 2000椭球的主要几何和物理参数,比较这些参数与GRS 80和WGS 84椭球相应参数之间的差异,给出CGCS 2000椭球与GRS 80及WGS 84椭球定义的正常重力值的差异,并分析在CGCS 2000及WGS 84系下同一点坐标的差异.研究表明:CGCS 2000椭球上的正常重力值与GRS 80,WGS 84椭球上的正常重力值的差值分别约为-143.54×10-8m/s2和0.02×10-8m/s2.同一点在CGCS 2000与GRS 80和WGS 84下经度相同,纬度的最大差值分别为8.26×10-11"(相当于2.5×10-6 mm)和3.6×10-6"(相当于0.11 mm). 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
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马家琼;杨晓英;崔文刚;陈涛;胡君 《东北测绘》2013,(4):158-160
伴随着坐标转换问题成为诸多项目研究热点,在进行不同国家坐标系以及国家坐标系与地方独立坐标系之间的坐标转换时问题层出不穷。通过坐标转换,实现了不同坐标系下数据与数据之间转换精度研究及影像与数据叠合精度分析。本文就WGS-84与西安80坐标转换问题进行探讨。 相似文献