排序方式: 共有66条查询结果,搜索用时 15 毫秒
51.
将方案评价与决策的思想引入到卫星链路配置中,建立了中继卫星链路参数配置的多目标模型,并用\"短板链路\"优先配置的原则,将多目标模型缩减为三目标模型。采用基于物理规划的决策方法,给出了决策三目标配置模型最优解的具体实现算法。通过实例分析表明该决策方法是可行的。 相似文献
52.
介绍美军现役主要战术数据链及美军针对四代机的数据链改进和试验情况,分析美军第四代战斗机的技战术性能,得到美军对下一代数据链建设方向的重点,对我军今后数据链建设具有借鉴意义,从而更有针对性地加强我军的数据链建设,提高我空军的整体战斗力。 相似文献
53.
54.
55.
56.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(8):1922-1940
Time-varying spherical harmonic coefficients determined from the Gravity Recovery and Climate Experiment (GRACE) data provide a valuable source of information about the water mass exchange that is the main contributor to the Earth’s gravity field changes within a period of less than several hundred years. Moreover, by measuring seawater temperature and salinity at different layers of ocean depth, Argo floats help to measure the steric component of global mean sea level (GMSL). In this study, we quantify the rate of barystatic sea-level change using both GRACE RL05 and RL06 monthly gravity field models and compare the results with estimates achieved from a GMSL budget closure approach. Our satellite altimetry-based results show a trend of 3.90 ± 0.14 mm yr−1 for the GMSL rise. About 35% or 1.29 ± 0.07 mm yr−1 of this rate is caused by the thermosteric contribution, while the remainder is mainly due to the barystatic contribution. Our results confirm that the choice of decorrelation filters does not play a significant role in quantifying the global barystatic sea-level change, and spatial filtering may not be needed. GRACE RL05 and RL06 solutions result in the barystatic sea-level change trends of 2.19 ± 0.13 mm yr−1 and 2.25 ± 0.16 mm yr−1, respectively. Accordingly, the residual trend, defined as the difference between the altimetry-derived GMSL and sum of the steric and barystatic components, amounts to 0.51 ± 0.51 and 0.45 ± 0.44 mm yr−1 for RL05 and RL06-based barystatic sea-level changes, respectively, over January 2005 to December 2016. The exclusion of the halosteric component results in a lower residual trend of about 0.36 ± 0.46 mm yr−1 over the same period, which suggests a sea-level budget closed within the uncertainty. This could be a confirmation on a high level of salinity bias particularly after about 2015. Moreover, considering the assumption that the GRACE-based barystatic component includes all mass change signals, the rather large residual trend could be attributed to an additional contribution from the deep ocean, where salinity and temperature cannot be monitored by the current observing systems. The errors from various sources, including the model-based Glacial Isostatic Adjustment signal, independent estimation of geocenter motion that are not quantified in the GRACE solutions, as well as the uncertainty of the second degree of zonal spherical harmonic coefficients, are other possible contributors to the residual trend. 相似文献
57.
Istvan Laszlo Pubu Ciren Hongqing Liu Shobha Kondragunta J. Dan Tarpley Mitchell D. Goldberg 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(11):1882-1893
The paper presents a high-level overview of current and future remote sensing of aerosol and shortwave radiation budget carried out at the US National Oceanic and Atmospheric Administration (NOAA) from the US Geostationary Operational Environmental Satellite (GOES) series. The retrievals from the current GOES imagers are based on physical principles. Aerosol and radiation are estimated in separate processing from the comparison of satellite-observed reflectances derived from a single visible channel with those calculated from detailed radiative transfer. The radiative transfer calculation accounts for multiple scattering by molecules, aerosol and cloud and absorption by the major atmospheric gases. The retrievals are performed operationally every 30 min for aerosol and every hour for radiation for pixel sizes of 4-km (aerosol) and 15- to 50-km (radiation). Both retrievals estimate the surface reflectance as a byproduct from the time composite of clear visible reflectances assuming fixed values of the aerosol optical depth. With the launch of GOES-R NOAA will begin a new era of geostationary remote sensing. The Advanced Baseline Imager (ABI) onboard GOES-R will offer capabilities for aerosol remote sensing similar to those currently provided by the Moderate Resolution Imaging Spectroradiometer (MODIS) flown on the NASA Earth Observing System (EOS) satellites. The ABI aerosol algorithm currently under development uses a multi-channel approach to estimate the aerosol optical depth and aerosol model simultaneously, both over water and land. Its design is strongly inspired by the MODIS aerosol algorithm. The ABI shortwave radiation budget algorithm is based on the successful GOES Surface and Insolation Product system of NOAA and the NASA Clouds and the Earth’s Radiant Energy System (CERES), Surface and Atmospheric Radiation Budget (SARB) algorithm. In all phases of the development, the algorithms are tested with proxy data generated from existing satellite observations and forward simulations. Final assessment of the performance will be made after the launch of GOES-R scheduled in 2012. 相似文献
58.
信道和链路干扰仿真是数据链测试仿真评估系统的关键技术之一。在局域网下模拟数据链系统真实运行的无线环境的非理想特性,需要对典型应用环境的信道条件、干扰特征进行分析和建模,仿真验证数据链系统在不同环境条件下的性能。本文首先分析了几类常见的信道和链路干扰仿真工具相关模块的原理和机制,研究并提出了传输时延、信道与链路干扰、链路级仿真方法及方案,并对几个关键问题进行了分析并提出解决方案。该研究在数据链测试仿真评估系统中的验证效果良好,能够为数据链系统可靠性、稳定性提供无线信道和链路干扰模拟工具,从而为数据链系统的设计提供参考和依据。 相似文献
59.
太阳风向磁层电离层(Magnetosphere and Ionosphere, MI)系统输入能量, 而输入的能量随后在MI系统中消耗. 本文从能量守恒原理出发, 讨论太阳风-磁层-电离层 (SMI)耦合过程中的能流路径和能量收支的定量关系. 主要讨论9个问题: (1) 太阳风向MI系统的能量输入, (2) MI系统对能量输入的响应, (3) 环电流的能量消耗, (4) 极区电离层焦耳加热的能量消耗, (5) 极光粒子沉降的能量消耗, (6) 磁尾能量的消耗、储存以及返回下游太阳风, (7)平静期间的能量积累与释放, (8)能量在不同能汇中的分配, (9)评价能量函数的准则和方法. 相似文献
60.