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691.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(8):1910-1921
Cadastral information of rice fields is important for monitoring cropping practices in Taiwan due to official initiatives. Remote sensing based rice monitoring has been a challenge for years because the size of rice fields is small, and crop mapping requires information of crop phenology, relating to spatiotemporal resolution of satellite data. This study aims to develop an approach for mapping rice-growing areas at field level using multi-temporal Sentinel-2 data in Taiwan. The data were processed for 2018, following four main steps: (1) construct time-series Enhanced Vegetation Index (EVI) and Land Surface Water Index (LSWI), (2) noise filtering of the time-series data using wavelet transform, (3) rice crop classification using information of crop phenology, and (4) parcel-based accuracy assessment of the mapping results. The parcel-to-parcel comparisons between mapping results and ground reference data indicated satisfactory results. These findings were confirmed by close agreement between satellite-derived rice area and government’s statistics. Although some factors, including mixed-pixel issues and cloud-cover effects, lowered the mapping accuracies of townships along the coastline, this study has demonstrated the efficacy of using multitemporal Sentinel-2 data to create a reliable database of rice-growing areas over a large and heterogeneous region. Such a quantitative information was important for updating rice crop maps and monitoring cropping practices. 相似文献
692.
以西锐SR2X飞机海外标准复装为例,初步探索了飞机技术出版物在通用飞机复装中的使用,明确了通用飞机复装的技术依据和作业流程,为未来通用飞机制造商或代理商复装飞机提供了工程经验。 相似文献
693.
Minakshi Devi A.K. Barbara Ko-Ichiro Oyama Chia-Hung Chen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The modifications induced in the dynamics of the ionosphere by the major Japan earthquake (EQ) of March 11, 2011 (epicenter at 38.322°N, 142.369°E, M = 8.9) in presence of a magnetic storm are examined by mapping latitudinal variations of F-layer ionization density (NmF2) from 22 stations covering the epicenter zone. The changes forced into the Total Electron Content (TEC) by the major EQ in the magnetic storm ambiance are also examined from the GPS data collected at Guwahati (26° 10′ N, 91° 45’ E), situated in the major fault system of East Asia. The contributions of pre-seismic electric field as well as of magnetic storm time electric field in the observed density variations are brought into the ambit of discussion. The influence of lower atmosphere in shaping TEC features during the study case is highlighted. The effects of solar activity on density variations during such complex ambiances are also addressed. 相似文献
694.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014,53(2):219-225
The Ionospheric F2-layer peak parameters response to a magnetic storm had been investigated over Ilorin, Nigeria (Lat. 8:53°N, Long. 4.5°E, dip angle, −2.96°), Jicamarca, Peru (11.95°S, 76.87°W, dip angle, 0.8°) and Hermanus, South Africa (34.42°S, 19.22°E, dip angle, −60.77°), using percentage enhancement/depletion values. Our results showed an enhancement in NmF2 at all of these stations. Averagely, pre-noon and post-noon peaks are highest at Ilorin during quiet time. The similar pattern observed for quiet condition between Ilorin and Jicamarca was due to their latitudinal positions. For disturbed NmF2 condition, Jicamarca and Ilorin recorded higher peaks at nighttime than during the daytime for the storms main phase, and the reverse over Hermanus. The nighttime and daytime increases were observed respectively at Ilorin and Hermanus during the recovery period. The hmF2 variation recorded higher enhancement at Jicamarca during the daytime and at Hermanus at nighttime during the main phase. During the recovery phase, the highest enhancement was recorded during the daytime at Jicamarca, and over Hermanus at nighttime. These observations find their explanation in the magnetospheric current, solar wind and E × B drift. 相似文献
695.
考虑到地球扁率J_2摄动的影响,在非正交分解法的基础上,利用自由段弹道地心距迭代解析解,给出了一种弹道飞行器零射程线的计算方法。数值仿真结果表明,该方法具有很高的精度,且计算速度较快,在闭路制导能量耗散和多弹头进攻弹道设计中具有较高的应用价值。 相似文献
696.
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698.
Nina Zolotukhina Nelya Polekh Olga Pirog 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Statistical and spectral analyses are performed to investigate variations of two ionosphere F2 layer key parameters, the critical frequency (foF2) and the peak height (hmF2), that were measured over Irkutsk (52.5°N, 104.0°E) from December 2006 to January 2008 under solar minimum. The analyses showed that both parameters contain quasi-harmonic oscillations with periods of Tn = 24/n hours (n = 1–7), among which the diurnal (n = 1) and semidiurnal (n = 2) ones are the strongest. Seasonal variations are explored of mean and median values, spectrum, amplitude, and phase of the diurnal and semidiurnal components of foF2 and hmF2. 相似文献
699.
提出一种散乱点云自适应滤波算法,该算法采用改进的R*-树组织散乱点云的拓扑近邻关系,基于该结构快速准确获取局部型面参考数据,自适应调节二维高斯分布的数字特征计算滤波权值,计算局部型面参考数据对原始型面数据的影响因子,以此作为权值计算各点滤波后的坐标,采用加权平均方法实现散乱点云的自适应滤波.实验证明该算法可有效提高点云的滤波效率,在保留原始型面特征的基础上,减小点云的随机误差,提高光顺性. 相似文献
700.
分辨率的不断提高对低轨遥感卫星的星地数据传输能力提升提出了迫切需求,导致X频段星地数传通道压力急剧增加,而Ka频段可用带宽是X频段的4倍,理论上可大幅提升传输能力。当前低轨遥感卫星的星地数据传输通常采用固定编码调制(CCM)和可变编码调制(VCM),均未利用地面站仰角增大时大气衰减减小所带来的信道条件改善,对链路资源造成浪费。针对此问题,对指定地面站和链路可用度,综合考虑自由空间损耗和大气衰减随接收仰角增加而同时减小的特性,提出基于DVB S2标准的Ka频段星上VCM系统实现方案,给出传输效能评估标准,并对降雨特性不同的喀什站、北京站、三亚站CCM,VCM的Ka频段传输效能进行了对比仿真分析,以寻找出适合不同站点的星地数传方案。仿真结果表明:干旱少雨的喀什站更适合采用CCM,且链路可用度高达99.82%;雨量中等的北京站可根据用户使用需求灵活选择CCM或VCM;而降雨丰富的三亚站更适合采用VCM,不仅可将传输效能提升8.37%,还可将链路可用度提升11.23%。 相似文献