Analysis of mapping coverage obtained from spacecraft     

Anastassios E. Petropoulos  James M. Longuski 《Celestial Mechanics and Dynamical Astronomy》1994,60(4):431-454

An exact analysis of the coverage obtained by spacecraft using cross-track scanning and nadir-centered conical imaging, under imposed viewing obliqueness and resolution requirements, is presented. In addition to exact expressions for the area acquired and the area acquisition rate, envelope theory is introduced to obtain the boundary of the imaged area. These expressions are relatively compact, allowing rapid machine computation. The effects of the sun phase angle, and of imaging system limitations are also examined. The Galileo mission encounter with Callisto is used as a numerical example, from which certain general conclusions are drawn regarding optimal imaging trajectories.  相似文献   

Observations with the Visual and Infrared Mapping Spectrometer (VIMS) during Cassini's flyby of Jupiter     

R.H. Brown  K.H. Baines  J.-P. Bibring  F. Capaccioni  R.N. Clark  D.P. Cruikshank  V. Formisano  Y. Langevin  T.B. McCord  V. Mennella  P.D. Nicholson  C. Sotin  M.A. Chamberlain  G. Hansen  M. Showalter 《Icarus》2003,164(2):461-470

The Cassini Visual and Infrared Mapping Spectrometer (VIMS) is an imaging spectrometer covering the wavelength range 0.3-5.2 μm in 352 spectral channels, with a nominal instantaneous field of view of 0.5 mrad. The Cassini flyby of Jupiter represented a unique opportunity to accomplish two important goals: scientific observations of the jovian system and functional tests of the VIMS instrument under conditions similar to those expected to obtain during Cassini's 4-year tour of the saturnian system. Results acquired over a complete range of visual to near-infrared wavelengths from 0.3 to 5.2 μm are presented. First detections include methane fluorescence on Jupiter, a surprisingly high opposition surge on Europa, the first visual-near-IR spectra of Himalia and Jupiter's optically-thin ring system, and the first near-infrared observations of the rings over an extensive range of phase angles (0-120°). Similarities in the center-to-limb profiles of H⁺₃ and CH₄ emissions indicate that the H⁺₃ ionospheric density is solar-controlled outside of the auroral regions. The existence of jovian NH₃ absorption at 0.93 μm is confirmed. Himalia has a slightly reddish spectrum, an apparent absorption near 3 μm, and a geometric albedo of 0.06±0.01 at 2.2 μm (assuming an 85-km radius). If the 3-μm feature in Himalia's spectrum is eventually confirmed, it would be suggestive of the presence of water in some form, either free, bound, or incorporated in layer-lattice silicates. Finally, a mean ring-particle radius of 10 μm is found to be consistent with Mie-scattering models fit to VIMS near-infrared observations acquired over 0-120° phase angle.  相似文献   

新世纪大洋钻探"三角鼎立"中的欧洲联合体     

刘玉柱  高月华 《海洋地质前沿》2002,18(5):19-20

欧洲为了与美国、日本在IODP中处于同等重要的地位，成立了由ODP成员参加的欧洲大洋钻探科学指导委员会（ESCOD）和JEODI组织，并开展了IODP之前的一系列准备活动。在其中的APLACON会议上，论证了IODP中第三类特定钻探平台的必要性，讨论了该类平台在某些研究范围内的重要作用，包括研究地球历史中的极端气候（北极海区）、重建白垩纪－第三纪的水文地理学、气候的快速变化、沉积盆地形成与过程以及固体地球过程等。  相似文献   

Outlier detection algorithms and their performance in GOCE gravity field processing   总被引：2，自引：0，他引：2  

M. Kern  T. Preimesberger  M. Allesch  R. Pail  J. Bouman  R. Koop 《Journal of Geodesy》2005,78(9):509-519

The satellite missions CHAMP, GRACE, and GOCE mark the beginning of a new era in gravity field determination and modeling. They provide unique models of the global stationary gravity field and its variation in time. Due to inevitable measurement errors, sophisticated pre-processing steps have to be applied before further use of the satellite measurements. In the framework of the GOCE mission, this includes outlier detection, absolute calibration and validation of the SGG (satellite gravity gradiometry) measurements, and removal of temporal effects. In general, outliers are defined as observations that appear to be inconsistent with the remainder of the data set. One goal is to evaluate the effect of additive, innovative and bulk outliers on the estimates of the spherical harmonic coefficients. It can be shown that even a small number of undetected outliers (<0.2 of all data points) can have an adverse effect on the coefficient estimates. Consequently, concepts for the identification and removal of outliers have to be developed. Novel outlier detection algorithms are derived and statistical methods are presented that may be used for this purpose. The methods aim at high outlier identification rates as well as small failure rates. A combined algorithm, based on wavelets and a statistical method, shows best performance with an identification rate of about 99%. To further reduce the influence of undetected outliers, an outlier detection algorithm is implemented inside the gravity field solver (the Quick-Look Gravity Field Analysis tool was used). This results in spherical harmonic coefficient estimates that are of similar quality to those obtained without outliers in the input data.  相似文献   

TRMM卫星微波成像仪分级产品及其反演降水算法   总被引：1，自引：2，他引：1  

邓伟何会中  程明虎崔哲虎 《气象科技》2004,32(4):206-212

文章叙述了获取定量降水信息的意义，简要介绍了对热带测雨卫星TRMM(Tropical Rainfall Measurement Mission)的仪器、美国国家宇航局提供的微波成像仪TMI(TRMM Microwave Imager)分级产品。对比了物理方法和经验方法反演降水的特点，并对一些经验方法以及倾斜对流系统对反演降水的影响、动态聚类分析、神经网络反演方法的研究成果进行了介绍。  相似文献   

On the effect of a low viscosity asthenosphere on the temporal change of the geoid—A challenge for future gravity missions     

Gabriele Marquart  Bernhard Steinberger  Karen Niehuus 《Journal of Geodynamics》2005,39(5):493

New satellite technology to measure changes in the Earth’s gravity field gives new possibilities to detect layers of low viscosity inside the Earth. We used density models for the Earth mantle based on slab history as well as on tomography and fitted the viscosity by comparison of predicted gravity to the new CHAMP gravity model. We first confirm that the fit to the observed geoid is insensitive to the presence of a low viscosity anomaly in the upper mantle as long as the layer is thin ( 200 km) and the viscosity reduction is less than two orders of magnitude. Then we investigated the temporal change in geoid by comparing two stages of slablet sinking based on subduction history or by advection of tomography derived densities and compared the spectra of the geoid change for cases with and without a low viscosity layer, but about equal fit to the observed geoid. The presence of a low viscosity layer causes relaxation at smaller wavelength and thus leads to a spectrum with relatively stronger power in higher modes and a peak around degrees 5 and 6. Comparing the spectra to the expected degree resolution for GRACE data for a 5 years mission duration shows a weak possibility to detect changes in the Earth’s gravity field due to large scale mantle circulation, provided that other causes of geoid changes can be taken into account with sufficient accuracy. A discrimination between the two viscosity cases, however, demands a new generation of gravity field observing satellites.  相似文献   

遥感与地球系统科学   总被引：1，自引：0，他引：1  

施建成  雷永荟 《遥感学报》2016,20(5):827-831

地球作为一个高度复杂的非线性系统,各圈层(大气、海洋、陆地、生物、冰雪圈、固体地球)尤其是人类活动等任何组成成份的变化,都会引起地球系统的变化。人类可持续发展面临的巨大科学挑战之一是认识人类赖以生存的、复杂变化的地球系统,认识地球系统如何变化及主要驱动因素,认识地球系统未来变化趋势及如何提高对全球变化的适应能力。卫星独特的全球覆盖和日尺度的观测改变了地球科学的研究方法,它强调所能探测到的多时空尺度上的物理动力过程,在全球范围应对气候变化、能源和环境挑战具有重要作用,揭开了地球系统多学科交叉的新纪元。以地球系统的视野,抓住驱动地球系统的关键循环过程(如能量、水、生物化学循环),是当前地球系统科学的发展趋势。地球系统科学(全球变化)研究需要长期稳定、准确性较高的卫星观测数据,以水循环为例,卫星遥感具备获取全球范围水循环关键参数能力,但是系统性综合观测能力不足,整体精确性受到综合化的可靠空间数据集的限制。目前中国正在积极研制发展新型水循环卫星WCOM(Water Cycle Observation Misssion),并寄希望以此为核心传感器发起全球分布式水循环观测星座系统,进一步提高中国在国际水循环观测与地球系统科学研究方面的话语权与领先能力。  相似文献   

Low Energy Transfer to the Moon   总被引：15，自引：0，他引：15  

W. S. Koon  M. W. Lo  J. E. Marsden  S. D. Ross 《Celestial Mechanics and Dynamical Astronomy》2001,81(1-2):63-73

In 1991, the Japanese Hiten mission used a low energy transfer with a ballistic capture at the Moon which required less Vthan a standard Hohmann transfer. In this paper, we apply the dynamical systems techniques developed in our earlier work to reproduce systematically a Hiten-like mission. We approximate the Sun–Earth–Moon-spacecraft 4-body system as two 3-body systems. Using the invariant manifold structures of the Lagrange points of the 3-body systems, we are able to construct low energy transfer trajectories from the Earth which execute ballistic capture at the Moon. The techniques used in the design and construction of this trajectory may be applied in many situations.  相似文献   

资源卫星（可见光）遥感数据获取任务调度优化算法研究   总被引：3，自引：0，他引：3  

徐雪仁  宫鹏  黄学智  金勇 《遥感学报》2007,11(1):109-114

从资源卫星（可见光）遥感数据获取任务调度的影响因子分析入手,在研究国外相关遥感任务调度算法的基础上,提出了基于目标的卫星遥感任务调度算法规则,并依据该规则研究建立了算法实现流程,以解决用户需求和星地资源使用约束之间的冲突,从而有效地满足用户对遥感数据的需求。  相似文献   

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郑伟  许厚泽  钟敏  刘成恕 《大地测量与地球动力学》2014,34(1):8-14

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