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同波束VLBI技术用于月球双探测器精密定轨及重力场解算 总被引:1,自引:0,他引:1
同波束VLBI通过同时观测两个探测器的多点频信号,可以得到两个探测器之间高精度的差分相位时延,日本月球探测计划SELENE充分体现了这一技术在月球探测器精密定轨中的贡献。本文针对采样返回的月球探测任务中,轨道器和返回器同时绕月飞行期间,研究利用同波束VLBI跟踪数据在探测器精密定轨和月球重力场仿真解算中的贡献。结果表明,加入同波束VLBI跟踪数据之后,探测器定轨精度有显著提高,改进超过一个量级。综合同波束VLBI跟踪数据解算得到的重力场模型相比于传统的USB双程测距测速数据,中低阶次位系数精度有明显改进,并且定轨精度有望能达到米级。
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Alexander F. Zakharov Francesco De Paolis Gabriele Ingrosso Achille Nucita Asghar Qadir 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(12):2061-2063
General relativity (GR) can be probed by several tests in the weak gravitational field limit. On the contrary, very poor information exists about GR tests in strong gravitational fields. Here, we focus on the interaction of light rays with the strong gravitational field of a massive black hole and show that relativistic images may form. Hence, we calculate the shapes of shadows (mirages) forming just near BH horizons and discuss the possibility to estimate the black hole parameters (mass, spin and charge) by future astrometric missions. In 2007, the Radioastron space telescope will be launched and it will allow to evaluate those parameters for the black hole hosted at the center of our Galaxy. 相似文献
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USB与VLBI联合确定“探测一号”卫星轨道 总被引:6,自引:0,他引:6
我国绕月探测工程“嫦娥一号”卫星将以统一S波段(USB)为主,辅以甚长基线干涉仪(VLB I)测轨分系统来完成测控任务。由于“探测一号”卫星轨道与“嫦娥一号”调相轨道段相似,有关单位于2005年3月17日—20日进行了USB和VLB I联合跟踪“探测一号”试验。通过对联合测轨数据的处理,研究了USB—VLB I联合定轨方法,分析了联合定轨和预报精度,得出了一些结论。 相似文献
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T. Hobiger M. SekidoY. Koyama T. Kondo 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Next-generation Very Long Baseline Interferometry (VLBI) system designs are aiming at 1 mm global position accuracy. In order to achieve this, it is not only necessary to deploy improved VLBI systems, but also to develop analysis strategies that take full advantage of the observations taken. Since the new systems are expected to incorporate four independent radio frequency bands, it should be feasible to resolve phase ambiguities directly from post-correlation data, providing roughly an order of magnitude improvement in precision of the delay observable. As the unknown ambiguities are of integer nature, it is discussed here how they the can be resolved analytically using algorithms which have been developed for Global Navigation Satellite System (GNSS) applications. Furthermore, it will be shown that ionosphere contribution and source structure effects, so-called core-shifts, can be solved simultaneously with the delay, which is the main geodetic observable for follow-on analysis. In order to verify the proposed algorithm, simulated observations were created using parameters from actual design studies. It is shown that, even in the case of low signal-to-noise ratio observations, reliable phase ambiguity resolution can be achieved and it is discussed how the integer ambiguity recovery depends on the number of observations and signal-to-noise ratio. 相似文献
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Katinka Geréb Sándor Frey 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The point source list of the Wilkinson Microwave Anisotropy Probe (WMAP) is a uniform, all-sky catalogue of bright sources with flux density measurements at high (up to 94 GHz) radio frequencies. We investigated the five-year WMAP list to compile a new catalogue of bright and compact extragalactic radio sources to be potentially studied with Very Long Baseline Interferometry at millimeter wavelengths (mm-VLBI) and Space VLBI (SVLBI). After comparing the WMAP data with the existing mm-VLBI catalogues, we sorted out the yet unexplored sources. Using the 41, 61 and 94 GHz WMAP flux densities, we calculated the spectral indices. By collecting optical identifications, lower-frequency radio flux densities and VLBI images from the literature, we created a list of objects which have not been investigated with VLBI at 86 GHz before. With total flux density at least 1 Jy and declination above −40°, we found 37 suitable new targets. It is a nearly 25% addition to the known mm-VLBI sources. Such objects are also potentially useful as phase-reference calibrators for the future Japanese SVLBI mission ASTRO-G at its highest observing frequency (43 GHz). The phase-referencing capability of ASTRO-G would allow long integrations and hence better sensitivity for observing faint target sources close to suitable phase calibrators in the sky. 相似文献
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针对地球静止轨道(GEO)卫星全天时全天候高精度的监测需求,考虑传统甚长基线干涉(VLBI)测站高成本、高投入和GEO卫星专用观测时段有限等制约条件,研发了简易型VLBI观测系统,并组建了包括上海、都匀和乌鲁木齐三站的微型VLBI网(micro VLBI network,MVN),开展了并置站测试以及对GEO卫星亚太6C的连续监测,并评估了当前MVN的观测能力。结果表明MVN扣除系统差后的单站接收精度为2ns,各基线观测时延拟后残差约几纳秒,GEO目标实测位置精度为百米级(内外符精度分别约100m和400m)。不同于传统VLBI和其他GEO监测手段,MVN还具备全天时、全天候、低造价、易布设及易推广等特点,充分表明了其在GEO卫星监测领域的应用价值。 相似文献