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1.
空间对地观测需求的增长和任务的多样性导致卫星区域覆盖分析变得越来越复杂。当前的遥感卫星区域覆盖算法与应用无法提供实时响应和应对高并发请求的在线服务,并且分析结果不能做到实时可视化,增加了数据的认知难度。针对于此,本文结合流式处理技术,提出一种高效的遥感卫星区域覆盖实时分析方法与可视化服务。首先,采用一种多模式判断策略,实现遥感卫星区域覆盖相关参数的高效计算;然后,对持续流入的数据进行实时分块,实现数据实时处理;最后,结合流式处理技术,提供实时响应和可视化的在线服务。利用多星多地面区域数据进行试验验证,结果表明,本文方法在保证传感器任意指向下遥感卫星区域覆盖参数计算精度的同时,效率得到较大提升,并且能够及时高效地通过数据流的方式,实现分析结果的实时可视化。 相似文献
2.
《制图学和地理信息科学》2013,40(1):7-15
State and local agencies involved in emergency response to natural disasters such as hurricanes have explicitly indicated they need imagery covering the disaster area within three days of the event; and more desirably within 24 hours of the event. Airborne image collections have often been used but suffer from several problems, most noticeably the collection time (days or week) required for larger areas. The use of remote sensing satellites carrying high spatial resolution sensors has often been touted as the logical response for rapidly collecting post-disaster event imagery for emergency response. Unfortunately, satellites are maintained on fixed orbits. The repeat interval for remote sensing satellites carrying high spatial resolution sensors, even with pointable sensors, is on the order of several days, depending on the latitude for the disaster event. Fortunately, more than one satellite carries high spatial resolution imagery. This combination of requirements and restrictions may result in either a relatively high (or low) likelihood of collecting imagery within the three-day window of opportunity. This research investigated the likelihood of collecting imagery over a hurricane disaster area based on the orbital cycles of three high spatial resolution imaging satellites. Using the spatial-temporal distribution of historic hurricane landfall locations as a proxy for the probability distribution of future hurricanes by latitude, the "visibility" of each landfall location to future satellite imaging opportunities was determined. The results indicate that the likelihood of collecting imagery within one day of the event varied between 17 and 39 percent by relying on one satellite image provider. However, if either of three satellite imagery sources (i.e., Ikonos-2, Quickbird-2, and Orbview-3) could be used, then the likelihood increased to 61 percent. By relying on three satellite imagery providers there is a likelihood of between 94 and 100 percent of collecting imagery within two or three days, respectively, after the event. 相似文献
3.
While the standardMercator projection / transverse Mercator projecton maps the equator / the transverse metaequator equivalent to the meridian of referenceequidistantly, theoblique Mercator projection aims at aconformal mapping of the ellipsoid of revolution constraint to anequidistant mapping of an oblique metaequator. Obliqueness is determined by the extension of the area to be mapped, e.g. determined by the inclination of satellite orbits: Satellite cameras map the area just under the orbit geometry. Here we derive themapping equations of theoblique Mercator projection being characterized to beconformal andequidistant on the oblique metaequator extending results ofM. Hotine (1946, 1947). 相似文献
4.
GNSS processing at CODE: status report 总被引:26,自引:19,他引:7
Rolf Dach Elmar Brockmann Stefan Schaer Gerhard Beutler Michael Meindl Lars Prange Heike Bock Adrian Jäggi Luca Ostini 《Journal of Geodesy》2009,83(3-4):353-365
Since May 2003, the Center for Orbit Determination in Europe (CODE), one of the analysis centers of the International GNSS Service, has generated GPS and GLONASS products in a rigorous combined multi-system processing scheme, which promises the best possible consistency of the orbits of both systems. The resulting products, in particular the satellite orbits and clocks, are easily accessible by the user community. In the first part of this article, we focus on the generation of the combined global products at CODE, where we put emphasis not only on accuracy, but also on completeness. We study the impact of GLONASS on the CODE products, and the benefit of using them. Last, but not least, we introduce AGNES (Automated GNSS Network for Switzerland), a regional tracking network of small extensions (roughly 400 km East–West, 200 km North–South), which consequently tracks all GNSS satellites and analyzes their measurements using the CODE products. 相似文献
5.
Guillaume Ramillien R. Biancale S. Gratton X. Vasseur S. Bourgogne 《Journal of Geodesy》2011,85(6):313-328
We propose an unconstrained approach to recover regional time-variations of surface mass anomalies using Level-1 Gravity Recovery
and Climate Experiment (GRACE) orbit observations, for reaching spatial resolutions of a few hundreds of kilometers. Potential
differences between the twin GRACE vehicles are determined along short satellite tracks using the energy integral method (i.e.,
integration of orbit parameters vs. time) in a quasi-inertial terrestrial reference frame. Potential differences residuals
corresponding mainly to changes in continental hydrology are then obtained after removing the gravitational effects of the
known geophysical phenomena that are mainly the static part of the Earth’s gravity field and time-varying contributions to
gravity (Sun, Moon, planets, atmosphere, ocean, tides, variations of Earth’s rotation axis) through ad hoc models. Regional
surface mass anomalies are restored from potential difference anomalies of 10 to 30-day orbits onto 1◦ continental grids by regularization techniques based on singular value decomposition. Error budget analysis has been made
by considering the important effects of spectrum truncation, the time length of observation (or spatial coverage of the data
to invert) and for different levels of noise. 相似文献
6.
7.
基于日地关系建立地影模型,利用数值法可以高精度计算单个卫星的地影参数,但是难以快速而全面地分析某一类卫星的地影参数变化和分布规律。本文从日、地和卫星三者的几何关系出发,提出了一种基于空间视场的卫星地影直接建模方法。首先,分别利用轨道半长轴和太阳的周年视运动确定卫星地影的大小和位置变化;其次,基于球面几何分析法推导了卫星地影参数的计算公式以及扁率摄动等对长期预报的影响改正公式。对北斗混合星座中3类卫星的地影参数分析试验表明,卫星地影模型和地影参数解析法能够快速获得中高轨近圆轨道类型的星蚀规律信息。 相似文献
8.
9.
A. Saalfeld 《Journal of Geodesy》1999,73(6):291-297
When a collection of double differences is used to compute global-positioning-system satellite orbits from a permanent network
of receiving stations, linear dependence among the double-differenced observations reduces the number of double differences
that contribute new information to the computations. A maximal linearly independent subset of a large collection of double
differences contains all the information content of the full set. If r is the number of receivers and s is the number of satellites, the original collection of double differences may have size O(r
2
s
2), whereas the linearly independent subset has size no greater than O(rs). Only such a smaller independent subset needs to participate in the more expensive double-precision matrix computations
to correctly correlate all double differences, detect cycle slips, resolve ambiguities, and compute satellite orbits and station
positions and relative velocities. Dependence among double differences is characterized using vector space methods together
with geometric characterizations of Boolean matrices. These characterizations lend themselves to fast, robust algorithms for
computing maximal linearly independent sets (bases) of double differences. An algorithm is given for constructing a generating
independent set of double differences from the Boolean array of receiving-station/satellite connections. Characterizations
of generator equivalence allow alternative generating sets to be identified and selected. An updating algorithm to handle
local changes in the satellite–receiver connection matrix is also described.
Received: 27 August 1996 / Accepted: 28 January 1999 相似文献
10.
一种基于标准纬线变更的瓦片索引方法 总被引:1,自引:0,他引:1
分析了常见的电子地图投影变形特征,提出了一种间断性变更标准纬线的非固定倍率瓦片索引方法。该方法在瓦片索引过程中,通过自动变更标准纬线来减小地图投影的变形程度。该方法在长度变形、角度变形和面积变形方面均具有整体变形较小的特点。在区域性电子地图表达中具有良好的变形可控性,具有较高的应用价值。 相似文献
11.
12.
卫星对侦查区域的覆盖语义是影响侦查覆盖效率的关键因素之一。针对现有覆盖算法低效耗时的技术瓶颈,提出了一种针对成像卫星区域覆盖的自适应规划方法,包括自适应的网格划分、平衡成像精度和覆盖效率的最大可视覆盖计算以及窗口优化的卫星区域覆盖策略。通过与常用经典算法对比,验证了本文方法的有效性和鲁棒性。本文方法已成功应用于某些在轨卫星的区域覆盖任务。 相似文献
13.
介绍了多组广播星历的轨道标准化的两种方法,通过对观测时段较长的同一GPS卫星多组广播星历分析,提出了整体轨道拟合方法进行GPS卫星轨道标准化,试验结果证明整体标准化方法优于分段标准化方法。 相似文献
14.
针对光学卫星成像时云导致的测区有效成像覆盖周期不确定问题,在卫星轨道计算的基础上,结合云量时空分布的历史统计规律、卫星历史观测数据的覆盖能力,研究建立光学卫星测区有效成像覆盖周期预估模型,回答测区有效成像覆盖效率与时间等问题,直接服务于光学卫星数据获取、产品生产和应用服务的计划安排和应用决策。 相似文献
15.
With the maturation of satellite technology,Hyperspectral Remote Sensing(HRS)platforms have developed from the initial ground-based and airborne platforms into spaceborne plat-forms,which greatly promotes the civil application of HRS imagery in the fields of agriculture,forestry,and environmental monitoring.China is playing an important role in this evolution,especially in recent years,with the successful launch and operation of a series of civil hyper-spectral spacecraft and satellites,including the Shenzhou-3 spacecraft,the Gaofen-5 satellite,the SPARK satellite,the Zhuhai-1 satellite network for environmental and resources monitoring,the FengYun series of satellites for meteorological observation,and the Chang'E series of spacecraft for planetary exploration.The Chinese spaceborne HRS platforms have various new characteristics,such as the wide swath width,high spatial resolution,wide spectral range,hyperspectral satellite networks,and microsatellites.This paper focuses on the recent progress in Chinese spaceborne HRS,from the aspects of the typical satellite systems,the data processing,and the applications.In addition,the future development trends of HRS in China are also discussed and analyzed. 相似文献
16.
The current low-cost global navigation satellite systems (GNSS) receiver cannot calculate satisfactory positioning results for pedestrian applications in urban areas with dense buildings due to multipath and non-line-of-sight effects. We develop a rectified positioning method using a basic three-dimensional city building model and ray-tracing simulation to mitigate the signal reflection effects. This proposed method is achieved by implementing a particle filter to distribute possible position candidates. The likelihood of each candidate is evaluated based on the similarity between the pseudorange measurement and simulated pseudorange of the candidate. Finally, the expectation of all the candidates is the rectified positioning of the proposed map method. The proposed method will serve as one sensor of an integrated system in the future. For this purpose, we successfully define a positioning accuracy based on the distribution of the candidates and their pseudorange similarity. The real data are recorded at an urban canyon environment in the Chiyoda district of Tokyo using a commercial grade u-blox GNSS receiver. Both static and dynamic tests were performed. With the aid of GLONASS and QZSS, it is shown that the proposed method can achieve a 4.4-m 1σ positioning error in the tested urban canyon area. 相似文献
17.
The adaptive composite map projection technique changes the projection to minimize distortion for the geographic area shown on a map. This article improves the transition between the Lambert azimuthal projection and the transverse equal-area cylindrical projection that are used by adaptive composite projections for portrait-format maps. Originally, a transverse Albers conic projection was suggested for transforming between these two projections, resulting in graticules that are not symmetric relative to the central meridian. We propose the alternative transverse Wagner transformation between the two projections and provide equations and parameters for the transition. The suggested technique results in a graticule that is symmetric relative to the central meridian, and a map transformation that is visually continuous with changing map scale. 相似文献
18.
19.
CODE’s five-system orbit and clock solution—the challenges of multi-GNSS data analysis 总被引:1,自引:1,他引:0
Lars Prange Etienne Orliac Rolf Dach Daniel Arnold Gerhard Beutler Stefan Schaer Adrian Jäggi 《Journal of Geodesy》2017,91(4):345-360
This article describes the processing strategy and the validation results of CODE’s MGEX (COM) orbit and satellite clock solution, including the satellite systems GPS, GLONASS, Galileo, BeiDou, and QZSS. The validation with orbit misclosures and SLR residuals shows that the orbits of the new systems Galileo, BeiDou, and QZSS are affected by modelling deficiencies with impact on the orbit scale (e.g., antenna calibration, Earth albedo, and transmitter antenna thrust). Another weakness is the attitude and solar radiation pressure (SRP) modelling of satellites moving in the orbit normal mode—which is not yet correctly considered in the COM solution. Due to these issues, we consider the current state COM solution as preliminary. We, however, use the long-time series of COM products for identifying the challenges and for the assessment of model-improvements. The latter is demonstrated on the example of the solar radiation pressure (SRP) model, which has been replaced by a more generalized model. The SLR validation shows that the new SRP model significantly improves the orbit determination of Galileo and QZSS satellites at times when the satellite’s attitude is maintained by yaw-steering. The impact of this orbit improvement is also visible in the estimated satellite clocks—demonstrating the potential use of the new generation satellite clocks for orbit validation. Finally, we point out further challenges and open issues affecting multi-GNSS data processing that deserves dedicated studies. 相似文献
20.
G. M. Appleby 《Journal of Geodesy》1998,72(6):333-342
In this paper we describe the results of an analysis of a 2.5-year set of satellite laser range observations of the two Etalon
geodetic satellites. We fit continuous orbits to the range observations, and map the range residuals into series of equivalent
orbital element residuals, considering in detail the orbital longitude, eccentricity and nodal residuals. We use the longitude
residuals to study thermal effects acting on the satellites and compare the results with those published for the Lageos satellites.
We discuss the differences between the two series of eccentricity residuals, and again compare the results with those from
Lageos. Finally we use the nodal residuals to investigate the potential for determination of UT1 of the reference frame defined
by the orbits of the Etalon satellites.
Received: 30 January 1997 / Accepted: 11 December 1997 相似文献