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381.
重力辅助惯性导航已渐成水下导航领域的研究热点,其实现是一项复杂的工程,涉及多项的关键技术.文章首先介绍了重力辅助导航的基本原理;之后详细阐述了在真实海洋环境下,重力辅助导航所需解决的若干关键技术问题,并给出了相应的研究成果;最后总结了我国水下重力辅助导航的发展趋势及研究的若干建议. 相似文献
382.
Mehdi Eshagh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The satellite gravity gradiometric data can be used directly to recover the gravity anomaly at sea level using inversion of integral formulas. This approach suffers by the spatial truncation errors of the integrals, but these errors can be reduced by modifying the formulas. It allows us to consider smaller coverage of the satellite data over the region of recovery. In this study, we consider the second-order radial derivative (SORD) of disturbing potential (Trr) and determine the gravity anomaly with a resolution of 1° × 1° at sea level by inverting the statistically modified version of SORD of extended Stokes’ formula. Also we investigate the effect of the spatial truncation error on the quality of inversion considering noise of Trr. The numerical investigations show satisfactory results when the area of Trr coverage is the same with that of the gravity anomaly and the integral formula is modified by the biased least-squares modification. The error of recovery will be about 6 mGal after removing the regularization bias in the presence of 1 mE noise in Trr measured on the orbit. 相似文献
383.
384.
论述了微波暗室静区反射率电平的测量方法和微波场强校准原理,分析了反射率电平对标准场法微波场强校准的影响。 相似文献
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空水界面声信号传播特性是水下检测空中声源首先要研究的问题,文中讨论了空中声源在水下产生声场的简正波模型,仿真分析了空中声源的水下声场,比较了简正波方法与射线方法、快速场方法对空中声源在水下产生的声场传播损失。结论表明简正波方法适用于远场传播损失。 相似文献
387.
O.S. Oyekola 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,43(12):1950-1956
Median values of ionosonde h′F data acquired at Ibadan (Geographic:7.4°N, 3.9°E, Magnetic: dip 6°S, and magnetic declination, 3°W), Nigeria, West Africa, have been used to determine vertical ion drift (electric field) characteristics in the postsunset ionosphere in the African region during a time of high solar activity (average F10.7 −208). The database spans from January and December 1958 during the era of International Geophysical Year (IGY) for geomagnetic quiet conditions. Bimonthly averaged diurnal variations patterns are very similar, but differ significantly in magnitude and in the evening reversal times. Also, monthly variations of F-region vertical ion drift reversal times inferred from the time of h′F maximum indicates early reversal during equinoxes and December solstice months except for the month of April. Late reversal is observed during the June solstice months. The equatorial evening prereversal enhancement in vertical ion drift (Vzp) occurs largely near 1900 LT with typical values 20–45 m/s. Comparison of Ibadan ionosonde Vzp with the values of prereversal peak velocity reported for Jicamarca (South America), Kodaikanal (India), and Scherliess and Fejer global model show considerable disparity. The changes of postsunset peak in virtual height of F-layer (h′FP) with prereversal velocity peak Vzp are anti-correlated. Investigation of solar effects on monthly values of Vzp and h′FP revealed that these parameters are independent of monthly averaged solar flux intensity during quiet-time sunspot maximum conditions. 相似文献
388.
基于标定场的激光雷达两步标定方法 《空间控制技术与应用》2017,43(4):57-62
针对激光雷达大测量范围高精度测角测距问题,提出一种基于标定场的激光雷达两步标定方法.该方法在分析激光雷达测角误差和测距误差的基础上,提出激光雷达误差修正模型.该模型将距离修正从标定模型中分离,首先利用靶标场完成全视场的角度标定,并确定其外部参数,再利用基线场实现距离标定.以降低距离标定参数与角度标定参数之间的耦合性,保证激光雷达角度和距离标定的精度和准确度.实验结果表明方法合理有效,能够实现激光雷达的高精度标定. 相似文献
389.
Carolus J. Schrijver 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
This review focuses on the processes that energize and trigger M- and X-class solar flares and associated flux-rope destabilizations. Numerical modeling of specific solar regions is hampered by uncertain coronal-field reconstructions and by poorly understood magnetic reconnection; these limitations result in uncertain estimates of field topology, energy, and helicity. The primary advances in understanding field destabilizations therefore come from the combination of generic numerical experiments with interpretation of sets of observations. These suggest a critical role for the emergence of twisted flux ropes into pre-existing strong field for many, if not all, of the active regions that produce M- or X-class flares. The flux and internal twist of the emerging ropes appear to play as important a role in determining whether an eruption will develop predominantly as flare, confined eruption, or CME, as do the properties of the embedding field. Based on reviewed literature, I outline a scenario for major flares and eruptions that combines flux-rope emergence, mass draining, near-surface reconnection, and the interaction with the surrounding field. Whether deterministic forecasting is in principle possible remains to be seen: to date no reliable such forecasts can be made. Large-sample studies based on long-duration, comprehensive observations of active regions from their emergence through their flaring phase are needed to help us better understand these complex phenomena. 相似文献
390.