基于数据融合的SRTM数据空洞填补方法   总被引：7，自引：0，他引：7  

阚瑷珂  朱利东  张瑞军  郑文锋  银正彤  王绪本  王成善 《地理空间信息》2007,5(3):62-64

总结国内外对SRTM数据空洞的填补方法,指出基于内插的填补方法无法满足大区域SRTM数据处理的需求。提出在内插的基础上进行数据融合的空洞填补方法,并以实例验证了该方法是一种获取完整地形数据的有效途径。  相似文献   

TRIFFID Photometry of Globular Cluster Cores — I. Photometric Techniques and Variable Stars in M15     

Butler  Shearer  Redfern  Colhoun  O'Kane  Penny  Morris  Griffiths  & Cullum 《Monthly notices of the Royal Astronomical Society》1998,296(2):379-391

The Galway/DIAS Image Sharpening Camera, TRIFFID, has been used to make observations in two colours of the centre of the post-core-collapse globular cluster M15. We present here our analysis of the photometry in B over two seasons. We have combined the complementary qualities of the HST 's high astrometric precision and TRIFFID's extended coverage and photometric precision, to perform crowded-field photometry in the innermost region of M15. Our technique virtually eliminates the problem of extreme crowding which has hitherto hampered studies of the variable star populations in globular cluster cores, and thereby provides an extension of the HST 's capability. Candidate variables detected with the HST have been confirmed and monitored over longer periods. We show that most of these are RR Lyrae stars, and that one is a short-period Type II Cepheid (the third to be discovered in M15). Our photometric study also produced evidence of a similar number of new variables. These also appear to be RR Lyrae stars, except for a possible eclipsing system. Further data from an upgraded version of TRIFFID have recently been obtained to help to refine the light curves of all these objects.  相似文献   

Sodium beacon tip–tilt determination with Rayleigh-aided auxiliary telescope technique     

S. Esposito  A. Riccardi  & R. Ragazzoni 《Monthly notices of the Royal Astronomical Society》1998,294(3):489-493

The usefulness of tracking the Rayleigh portion of a mesospheric sodium laser guide star as reference for absolute tip–tilt recovery in the frame of the auxiliary telescopes technique is shown. This approach leads to the reduction of the ground occupation needed to attain a given sky coverage by more than one order of magnitude. Speed, tracking precision, and the number of auxiliary telescopes are also reduced, making this new approach a more attractive one. The use of a low-altitude Rayleigh spot reinforces the fundamental limitations affecting this and other techniques, thus degrading significantly the quality of the recovered tip–tilt. However, it is shown that, provided adequate care is taken in the collection and treatment of data, an interesting tilt signal can still be retrieved.  相似文献   

The UVX quasar optical luminosity function and its evolution     

Pippa Goldschmidt  & Lance Miller 《Monthly notices of the Royal Astronomical Society》1998,293(1):107-112

The recently finished Edinburgh UVX quasar survey at B <18 is used together with other complete samples to estimate the shape and evolution of the optical luminosity function in the redshift range 0.3< z <2.2. There is a significantly higher space density of quasars at high luminosity and low redshift than previously found in the PG sample of Schmidt & Green, with the result that the shape of the luminosity function at low redshifts ( z <1) is seen to be consistent with a single power law. At higher redshifts the slope of the power law at high luminosities appears to steepen significantly. There does not appear to be any consistent break feature which could be used as a tracer of luminosity evolution in the population.  相似文献   

Proper motions and variability of the H₂ knots in the HH 111 and 121 protostellar outflows     

Kristen E. K. Coppin  Christopher J. Davis  & Milena Micono 《Monthly notices of the Royal Astronomical Society》1998,301(1):L10-L14

We discuss the formation of spectral features in the decelerating ejecta of gamma-ray bursts, including the possible effect of inhomogeneities. These should lead to blueshifted and broadened absorption edges and resonant features, especially from H and He. An external neutral ISM could produce detectable H and He, as well as Fe X-ray absorption edges and lines. Hypernova scenarios may be diagnosed by Fe Kα and H Lyα emission lines.  相似文献   

High-redshift galaxies in the Hubble Deep Field— II. Colours and number counts     

Lucia Pozzetti  Piero Madau  Gianni Zamorani  Henry C. Ferguson  & Gustavo Bruzual A. 《Monthly notices of the Royal Astronomical Society》1998,298(4):1133-1144

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Mapping on the HEALPix grid     

Mark R. Calabretta  Boudewijn F. Roukema 《Monthly notices of the Royal Astronomical Society》2007,381(2):865-872

The natural spherical projection associated with the Hierarchical Equal-Area and Isolatitude Pixelization (HEALPix) is described and shown to be one of a hybrid class that combines the cylindrical equal-area and Collignon projections, not previously documented in the cartographic literature. Projection equations are derived for the class in general and are used to investigate its properties. It is shown that the HEALPix projection suggests a simple method of (i) storing and (ii) visualizing data sampled on the grid of the HEALPix pixelization, and also suggests an extension of the pixelization that is better suited for these purposes. Potentially useful properties of other members of the class are described, and new triangular and hexagonal pixelizations are constructed from them. Finally, the standard formalism is defined for representing the celestial coordinate system for any member of the class in the FITS data format.  相似文献   

黄土填方区地表沉降时序InSAR监测分析     

王建业  梁小龙  金喜  白泽朝  齐二恒 《测绘通报》2021,(8):158-161

“削山填沟造地”等岩土工程在湿陷性黄土沟壑地区屡见不鲜,掌握填方区沉降情况具有重要意义。本文收集了2017年11月—2020年12月获取的56景TerraSAR-X StripMap模式影像,利用时序InSAR技术监测了陕北某湿陷性黄土填方地基工程的沉降信息,并与2017年11月—2020年12月期间监测区3个水准点的沉降测量结果比对。结果表明,在填方区地表以沉降为主,在挖方区地表以抬升为主,研究区存在有1处较为明显的地表沉降情况,位于填挖边界线附近填方区内,形变速率范围为-40~-20 mm/a,最大形变速率达-49.9 mm/a,累计量为-151.6 mm,时序InSAR形变结果和实地水准结果吻合性较好,垂直方向形变速率中误差为1.8 mm/a,表明时序InSAR技术在湿陷性黄土填挖方区变形监测中具有较好的应用价值。  相似文献   

基于图形分割的面状符号自动填充算法     

寇媛  姚炎林  王军军 《测绘地理信息》2021,46(2):93-95

针对现有制图软件在面状符号填充方面存在的符号缺失、压盖等问题,提出了一种基于图形分割的面状符号自动填充算法。该算法通过计算面的骨架线,对复杂面进行分解,判断分解后的简单面的形状,分别赋予不同的制图表达规则,实现面状符号的自动填充。结果表明,该算法可以有效实现狭长以及包含狭长分支的不规则图形的合理填充,有效解决了填充符号与图形边界、注记的压盖问题,提高了制图自动化,大大减少了制图工作量。  相似文献   

Finding the most variable stars in the Orion Belt with the All Sky Automated Survey     

J.A. Caballero  M. Cornide  E. de Castro 《Astronomische Nachrichten》2010,331(3):257-273

We look for high‐amplitude variable young stars in the open clusters and associations of the Orion Belt. We use public data from the ASAS‐3 Photometric V ‐band Catalogue of the All Sky Automated Survey, infrared photometry from the 2MASS and IRAS catalogues, proper motions, and the Aladin sky atlas to obtain a list of the most variable stars in a survey area of side 5° centred on the bright star Alnilam (ε Ori) in the centre of the Orion Belt. We identify 32 highly variable stars, of which 16 had not been reported to vary before. They are mostly variable young stars and candidates (16) and background giants (8), but there are also field cataclysmic variables, contact binaries, and eclipsing binary candidates. Of the young stars, which typically are active Herbig Ae/Be and T Tauri stars with Hα emission and infrared flux excess, we discover four new variables and confirm the variability status of another two. Some of them belong to the well known σ Orionis cluster. Besides, six of the eight giants are new variables, and three are new periodic variables (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献