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401.
模糊度解算是实现快速、高精度定位的关键,一直是全球卫星导航系统研究的热点。北斗系统提供三频信号,可以进行不同形式的组合,实现高精度定位和模糊度解算。通过分析现有的无电离层三频模糊度解算方法(TCAR)和组合观测值的噪声特征,提出一种低噪声无电离层影响的宽巷与IF组合相结合的TCAR算法,选取低噪声长波长的宽巷组合观测值,在几何模型下用最小二乘法逐级解算模糊度,最终实现静态定位。为了验证组合噪声的影响和各种TCAR算法的性能,对北斗中基线的实测数据进行实验,并且比较提出方法与现有算法的模糊度解算情况及位置精度。结果表明,提出方法可以有效提高模糊度解算的成功率,实现高精度定位。 相似文献
402.
以甲基三甲氧基硅烷(MTMS)和二甲基二甲氧基硅烷(DMDMS)为前驱体,通过溶胶-凝胶、常压干燥制备出柔性有机硅气凝胶,研究了MTMS与DMDMS的摩尔比对其化学组成和微观结构的影响;采用莫来石纤维毡作为增强体,制备出密度为0.25 g/cm~3的柔性有机硅气凝胶复合材料。实验结果表明,所制复合材料具有优异的热稳定性,其室温热导率在0.03 W/(m·K)以内;当MTMS和DMDMS的摩尔比为3.8∶1.2时,复合材料的均匀伸长率达3.6%、残重率达82.4%;复合材料经高温处理后,有机硅气凝胶转变为无机SiO_2气凝胶,较好地保持煅烧前的微观形貌和隔热性能;通过500 s石英灯静态加热,发现复合材料的表面有陶瓷化反应,厚度方向无收缩,背部温升81℃,表现出烧蚀/隔热的双重特性。 相似文献
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405.
通常使用无电离层(IF)线性组合(LC)消除低地球轨道(LEO)卫星简化动力学精密定轨(POD)一阶电离层延迟误差,忽略了高阶电离层(HOI)延迟误差。随着LEO卫星POD技术的发展,计算不同轨道高度的HOI延迟并探索其变化已成为进一步提高POD精度的重要手段。首先,使用国际参考电离层-2016(IRI-2016)和国际地磁参考场第13代(IGRF-13)模型,计算电离层穿刺点(IPP)位置和地磁场强度。其次,使用平滑星载GNSS数据计算电离层斜路径总电子含量(STEC)。然后,分别计算GOCE、GRACE-A和SWARM-A/B卫星的二阶和三阶电离层延迟。最后,评估了HOI延迟对LEO卫星重叠轨道分析、卫星激光测距(SLR)检核和精密科学轨道(PSO)比较结果的影响。实验结果表明:HOI延迟对LEO卫星简化动力学POD的影响大约在毫米至厘米的数量级上;HOI延迟对LEO卫星简化动力学POD外符合精度的影响分别达到0.92,0.22,0.21和0.18 mm;随着LEO卫星轨道高度的增加,HOI延迟对LEO卫星简化动力学POD的影响减小。 相似文献
406.
407.
Two central issues in magnetospheric research are understanding the mapping of the low-altitude ionosphere to the distant regions of the magnetsphere, and understanding the relationship between the small-scale features detected in the various regions of the ionosphere and the global properties of the magnetosphere. The high-latitude ionosphere, through its magnetic connection to the outer magnetosphere, provides an important view of magnetospheric boundaries and the physical processes occurring there. All physical manifestations of this magnetic connectivity (waves, particle precipitation, etc.), however, have non-zero propagation times during which they are convected by the large-scale magnetospheric electric field, with phenomena undergoing different convection distances depending on their propagation times. Identification of the ionospheric signatures of magnetospheric regions and phenomena, therefore, can be difficult. Considerable progress has recently been made in identifying these convection signatures in data from low- and high-altitude satellites. This work has allowed us to learn much about issues such as: the rates of magnetic reconnection, both at the dayside magnetopause and in the magnetotail; particle transport across the open magnetopause; and particle acceleration at the magnetopause and the magnetotail current sheets. 相似文献
408.
Energetic (0.1-16 keV/e) ion data from a plasma composition experiment on the ISEE-1 spacecraft show that Earth's plasma sheet (inside of 23 RE) always has a large population of H+ and He++ ions, the two principal ionic components of the solar wind. This population is the largest, in terms of both number density and spatial thickness, during extended periods of northward interplanetary magnetic field (IMF) and is then also the most "solar wind-like" in the sense that the He++/H+ density ratio is at its peak (about 3% on average in 1978 and 79) and the H+ and He++ have mean (thermal) energies that are in the ratio of about 1:4 and barely exceed the typical bulk flow energy in the solar wind. During geomagnetically active times, associated with southward turnings of the IMF, the H+ and He++ are heated in the central plasma sheet, and reduced in density. Even when the IMF is southward, these ions can be found with lower solar wind-like energies closer to the tail lobes, at least during plasma sheet thinning in the early phase of substorms, when they are often seen to flow tailward, approximately along the magnetic field, at a slow to moderate speed (of order 100 km s-1 or less). These tailward flows, combined with the large density and generally solar wind-like energies of plasma sheet H+ and He++ ions during times of northward IMF, are interpreted to mean that the solar wind enters along the tail flanks, in a region between the lobes and the central plasma sheet, propelled inward by ExB drift associated with the electric fringe field of the low latitude magnetopause boundary layer (LLBL). In order to complete this scenario, it is argued that the rapid (of order 1000 km s-1) earthward ion flows (mostly H+ ions), also along the magnetic field, that are more typically the precursors of plasma sheet "recovery" during substorm expansion, are not proof of solar wind entry in the distant tail, but may instead be a time-of-flight effect associated with plasma sheet redistribution in a dipolarizing magnetic field. 相似文献
409.
低温成型 Nomex蜂窝 U型夹层板研制 总被引:2,自引:0,他引:2
低温成型U型峰窝夹层板是一种新开发的低成本成型工艺。本文研究了木模成型环氧玻璃钢面板、Nomex峰窝芯U型夹层结构航空制件的三步骤工艺方案,分析解决了板芯粘接性能、抗压强度、重量控制的低温成型工艺难点。 相似文献
410.
张新航%李强%赵荣%张海鹏%张崇耿 《宇航材料工艺》2005,35(1):39-41
采用过氧化物硫化体系,芳纶纤维和耐烧蚀树脂作为耐烧蚀填料,阻燃剂为无卤的含磷阻燃剂,并通过L9(3^3)正交实验确定了含磷阻燃剂、耐烧蚀树脂、气相二氧化硅的最佳用量分别为25份、15份、15份。确定最佳配方和工艺生产出的三元乙丙橡胶绝热层密度为1.06—1.07g/cm^3,线烧蚀率为0.099mm/s,质量烧蚀率为0.043g/s,满足了某固体火箭发动机燃烧室内壁绝热层的技术要求。 相似文献