基于小波分析的线状要素压缩优化的综合性研究     

王玉海  朱长青 《武汉大学学报(信息科学版)》2007,32(7):630-632,653

利用小波分析理论、Douglas算法、曲率分析算法，对线状要素的压缩优化进行了深入的研究，并在建立线状要素压缩优化的自适应模型的基础上，对实际数据进行了试验。结果表明，此方法不仅能够保持高的压缩比，而且能够很好地保持原数据的特征。  相似文献   

2004年9月川渝大暴雨期间西南低涡结构及其环境场的分析   总被引：11，自引：1，他引：11  

赵思雄  傅慎明 《大气科学》2007,31(6):1059-1075

采用NCEP再分析资料、常规观测资料、卫星云图资料及地面降水资料, 对2004年9月2日～8日发生在川东和重庆的大暴雨的影响系统及其环境场作了分析研究。结果表明, 此次暴雨分为三个阶段, 降水系统主要有两个:第一、三阶段的主要降水系统是低空切变线；第二阶段的主要降水系统是西南低涡, 而西南低涡影响期内的雨量最强、范围最大。西南低涡开始时为一β中尺度系统, 最后发展达α中尺度系统。其影响时间从4日00时到6日06时 (国际协调时）, 持续了54小时。本文对此次暴雨过程所做的研究表明, 川东地区的特殊地形, 500 hPa高空小槽以及700 hPa、 850 hPa低层鞍型流场均是西南低涡产生和维持的重要条件； 西南低涡上层为暖性结构； 在暴雨过程中有20个雨团接连发生, 中尺度系统是这次暴雨的直接影响系统；对水汽收支的计算表明, 水汽可能来自于低纬度热带地区。本文还对西南低涡与东北低涡的异同作了比较。  相似文献   

Reprocessed emission line profiles from dense clouds in geometrically thick accretion engines     

Sean A. Hartnoll  Eric G. Blackman 《Monthly notices of the Royal Astronomical Society》2001,324(1):257-266

The central engines of active galactic nuclei (AGN) contain cold, dense material as well as hot X-ray-emitting gas. The standard paradigm for the engine geometry is a cold thin disc sandwiched between hot X-ray coronae. Strong support for this geometry in Seyferts comes from the study of fluorescent iron line profiles, although the evidence is not ubiquitously airtight. The thin disc model of line profiles in AGN and in X-ray binaries should still be benchmarked against other plausible possibilities. One proposed alternative is an engine consisting of dense clouds embedded in an optically thin, geometrically thick X-ray-emitting engine. This model is also motivated by studies of geometrically thick engines such as advection-dominated accretion flows (ADAFs). Here we compute the reprocessed iron line profiles from dense clouds embedded in geometrically thick, optically thin X-ray-emitting discs near a Schwarzschild black hole. We consider a range of cloud distributions and disc solutions, including ADAFs, pure radial infall and bipolar outflows. We find that such models can reproduce line profiles similar to those from geometrically thin, optically thick discs and might help alleviate some of the problems encountered from the latter. Thus, independent of thin discs, thick disc engines can also exhibit iron line profiles if embedded dense clouds can survive long enough to reprocess radiation.  相似文献   

Short-period line profile variations in the Be star ε Cap     

L. A. Balona  W. A. Lawson 《Monthly notices of the Royal Astronomical Society》2001,321(1):131-142

We present new high-dispersion spectroscopic data for the Be star ε Cap. The purpose of these data is to study the short-period line profile variations. By using a two-dimensional period-finding technique, we confirm that the photometric period of 0.99 d is present in the helium line profiles. We show that the variations are not easily explained by non-radial pulsation and suggest that corotating circumstellar material is responsible.  相似文献   

Monitoring Changes of Ice Streams Using Time Series of Satellite-Altimetry-Based Digital Terrain Models     

Ute C. Herzfeld  Craig S. Lingle  Cecily Freeman  Chris A. Higginson  Michael P. Lambert  Li-Her Lee  Vera A. Voronina 《Mathematical Geology》1997,29(7):859-890

The Antarctic Ice Sheet plays a major role in the global system, and the large ice streams discharging into the circumpolar sea represent its gateways to the world's oceans. Satellite radar altimeter data provide an opportunity for mapping surface elevation at kilometer-resolution with meter-accuracy. Geostatistical methods have been developed for the analysis of these data. Applications to Seasat data and data from the Geosat Exact Repeat Mission indicate that the grounding line of Lambert Glacier/Amery Ice Shelf, the largest ice stream in East Antarctica, has advanced 10–12 km between 1978 and 1987–89. The objectives of this paper are to explore possibilities and limitations of satellite-altimetry-based mapping to capture changes for shorter time windows and for smaller areas, and to investigate some methodological aspects of the data analysis. We establish that one season of radar altimeter data is sufficient for constructing a map. This allows study of interannual variation and is the key for a time-series analysis approach to study changes in ice streams. Maps of the lower Lambert Glacier and the entire Amery Ice Shelf are presented for austral winters 1978, 1987, 1988, and 1989. As a first step toward understanding the dynamics of the ice-stream/ice-shelf system, elevation changes are calculated for grounded ice, the grounding zone, and floating ice. In the absence of (sufficient) surface gravity control for the Lambert Glacier/Amery Ice Shelf area, altimetry-based maps may facilitate improvement of geoid models as they provide constraints on the terrain correction in the inverse gravimetric problem.  相似文献   

Carbon recombination lines from the Galactic plane at 34.5 & 328 MHz     

N. G. Kantharia  K. R. Anantharamaiah 《Journal of Astrophysics and Astronomy》2001,22(1):51-80

We present the results of a search for carbon recombination lines in the Galaxy at 34.5 MHz (C575α) made using the dipole array at Gauribidanur near Bangalore. Observations made towards 32 directions resulted in detections of lines, in absorption at nine positions. Followup observations at 328 MHz (C272α) using the Ooty Radio Telescope detected these lines in emission. A VLA D-array observation of one of the positions at 330 MHz yielded no detection implying a lower limit of 10′ for the angular size of the line forming region. The longitude-velocity distribution of the observed carbon lines indicate that the line forming regions are located mainly between 4 kpc and 7 kpc from the Galactic centre. Combining our results with published carbon recombination line data near 76 MHz (Erickson, McConnell & Anantharamaiah 1995), we obtain constraintson the physical parameters of the line forming regions. We find thatif the angular size of the line forming regions is ≥ 4°, then the range of parameters that fit the data are:T _e =20–40 K,n _e ∼ 0.1–0.3 cm⁻³ and pathlengths ∼ 0.07–0.9 pc which may correspond to thin photodissociated regions around molecular clouds. On the other hand, if the line forming regions are ∼ 2° in extent, then warmer gas (T _e ∼ 60–300 K) with lower electron densities (n _e ∼ 0.03–0.05 cm⁻³) extending over several tens of parsecs along the line of sight and possibly associated with atomic HI gas can fit the data. Based on the range of derived parameters, we suggest that the carbon line regions are most likely associated with photo-dissociation regions.  相似文献   

Spectrophotometric observations of a peculiar nitrogen-rich planetary nebula NGC 2440     

R. Louise 《Journal of Astrophysics and Astronomy》1982,3(2):145-150

By using the Boller and Chivens spectrograph with a moderate dispersion (59 å mm^-1) in the red spectral region, we obtained 65 spectra covering the whole surface of the planetary nebula NGC 2440. Intensities of Hα, [N II] λλ 6548–6584 and [S II] λλ 6717–6731 lines are derived using the IDS system available at the ESO in La Silva (Chile). The nebula is known to be a nitrogen-rich nebula (Peimbert 1978) surrounded by secondary structures (Minkowski 1964). The unusual high value of the [N II]/Hα in the central core (~ 30) is certainly due to the nitrogen overabundance occurring in that part of the nebula. Its variations from scale ionization structure (Capriotti, Cromwell and Williams 1971). The observations show clearly an outward increase of both [NII]/Hα andI(6717)/I(6713) ratios.  相似文献   

3DS在公路选线中的应用   总被引：1，自引：1，他引：0  

奥勇  王来录 《地球科学与环境学报》2004,26(4):63-66

基于3DS的公路选线分析系统．将GIS、遥感等技术引入公路建设工程的可行性分析中．充分发挥其数据可视化、空间分析等功能，从三维的角度和环境因素综合分析后做出公路选线的方案，有效地解决传统方法中的不足．加强分析过程的科学性，提高分析结果的准确性，缩短工作周期，大大提高工作效率。  相似文献   

Molecular Line Parameters for the “MASTER” (Millimeter Wave Acquisitions for Stratosphere/Troposphere Exchange Research) Database     

A.?PerrinEmail author  C.?Puzzarini  J.-M.?Colmont  C.?Verdes  G.?Wlodarczak  G.?Cazzoli  S.?Buehler  J.-M.?Flaud  J.?Demaison 《Journal of Atmospheric Chemistry》2005,51(2):161-205

In order to investigate the upper troposphere/lower stratosphere (UTLS) region of the earth's atmosphere, ESA/ESTEC (European space agency) is considering the opportunity to develop the spaceborne limb sounding millimeter sensor “MASTER” (millimeter wave acquisitions for stratosphere/troposphere exchange research). This instrument is part of the “atmospheric composition explorer for chemistry and climate interactions” (ACECHEM) project. In addition, ESA/ESTEC is developing the “MARSCHALS” (millimeter-wave airborne receiver for spectroscopic characterization of atmospheric limb sounding) airborne instrument which will demonstrate the feasibility of MASTER. The present paper describes the line-by-line database which was generated in order to meet at best the needs of the MASTER (or MARSCHALS) instrument. The linelist involves line positions, line intensities, line broadening and line shift parameters in the 294–305, 316–325, 342–348, 497–506 and 624–626 GHz spectral microwindows. This database was first generated for the target molecules for MASTER (H₂O, O₃, N₂O, CO, O₂, HNO₃, HCl, ClO, CH₃Cl, BrO). In addition, ten additional molecules (SO₂, NO₂, OCS, H₂CO, HOCl, HCN, H₂O₂, COF₂, HO₂ and HOBr) had also to be considered in the database as “possible interfering species” for the retrieval of the target molecules of MASTER. The line parameters were derived, depending on their estimated accuracy, (i) from a combination of spectral parameters included in the JPL and HITRAN catalogs (ii) from data taken into the literature or (iii) using data obtained through experimental measurements (and/or) calculations performed during the present study.  相似文献   

地震趋势预测的一种新模型研究   总被引：5，自引：0，他引：5  

康春丽刘德富  杜建国 《地球信息科学学报》2001,3(1):43-45

 本文根据自激励门限自回归模型原理,对多年的地震活动形势进行了分析,建立了用于地震大形势分析的客观化数值预测模式-在线预测模型。根据1980年以来中国大陆实际发生的地震资料对这一模型的可靠性进行了检验。统计结果表明,利用在线预测模型在对未来地震趋势进行预测时,其年度形势特征量的最大误差为0.3,平均误差为0.12;因此该模型能够比较客观地反映地震形势变化的自然特征及规律,较好的预测未来的地震活动趋势。这一模型的建立为促进地震趋势向客观化、定量化预测方向发展,提供了一种科学途径  相似文献