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装备时延校准误差是靶场测控系统中事件记录和交会定位的重要误差因素,其精确校准是实现装备时间同步的关键技术。针对装备时延问题展开研究,提出了一种物理含义清晰、易于测量的装备时延定义,实现了离散站点装备时延校准,验证了基于改进型B码的装备时延校准监控的有效性。试验结果表明,时延校准的精度达到了十微秒量级。 相似文献
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Siavash Iran Pour Tilo Reubelt Nico Sneeuw 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
Drawing on experience from Gravity Recovery and Climate Experiment (GRACE) data analysis, the scientific challenges were already identified in several studies. Any future mission should focus on improvement in both precision and resolution in space and time. For future gravity missions which use high quality sensors, aliasing of high frequency time-variable geophysical signals to the lower frequency signals is one of the most serious problems. The aliasing problem and the spatio-temporal resolution are mainly restricted by two sampling theorems describing the space-time sampling of satellite missions: (i) a Heisenberg-like uncertainty theorem which states that the product of spatial resolution and time resolution is constant, and (ii) the Colombo–Nyquist rule (CNR), which requires the number of satellite revolutions in a repeat period to be at least twice a given maximum spherical harmonic degree. The CNR holds under the assumption of equal ground-track spacing, and limits the spatial resolution of the gravity solution. 相似文献
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B. Andonov P. MukhtarovD. Pancheva 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The paper presents an empirical model of the total electron content (TEC) response to the geomagnetic activity described by the Kp-index. The model is built on the basis of TEC measurements covering the region of North America (50°W–150°W, 10°N–60°N) for the period of time between October 2004 and December 2009. By using a 2D (latitude-time) cross-correlation analysis it is found that the ionospheric response to the geomagnetic activity over the considered geographic region and at low solar activity revealed both positive and negative phases of response. The both phases of the ionospheric response have different duration and time delay with respect to the geomagnetic storm. It was found that these two parameters of the ionospheric response depend on the season and geographical latitude. The presence of two phases, positive and negative, of the ionospheric response imposed the implementation of two different time delay constants in order to properly describe the two different delayed reactions. The seasonal dependence of the TEC response to geomagnetic storms is characterized by predominantly positive response in winter with a short (usually ∼5–6 h) time delay as well as mainly negative response in summer with a long (larger than 15 h) time delay. While the TEC response in March and October is more close to the winter one the response in April and September is similar to the summer one. 相似文献
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