PRIMA for the VLTI – Science     

F. Delplancke  F. Derie  F. Paresce  A. Glindemann  F. Lévy  S. Lévêque  S. Ménardi 《Astrophysics and Space Science》2003,286(1-2):99-104

The four main scientific objectives of PRIMA – the Phase-Referenced Imaging and Micro-arc second Astrometry facility for the VLTI – will be described:– extra-solar system characterization with astrometry, to detect planets and evaluate their mass, and imaging of the dust accretion disk,– galactic center study with astrometry(dynamics of the bulge stars) and imaging at 10μm (piercing the gas and dust clouds surrounding the galactic center),– observations of AGNs and other extra-galactic objects, too faint to be observed without PRIMA, for which partial imaging is needed to constrain their structuremodels,– micro-gravitational lensing event resolution (imaging and astrometry of their photo-center) in the Galactic Bulge and Magellanic Clouds, helping to determine directly the lens mass and distance. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

用卫星高光谱数据提取德兴铜矿区植被污染信息   总被引：24，自引：7，他引：17  

刘圣伟  甘甫平  王润生 《国土资源遥感》2004,15(1):6-10,31

在深入分析研究德兴铜矿矿区植被光谱特征的基础上,利用美国EO-1卫星Hyperion高光谱数据,通过反演表征植物生理状态的光谱特征参数(红边位置和最大吸收深度)变异,提取与污染相关的信息,获取了矿山植被污染生态效应概况,为矿山污染的诊断和监测提供新技术和知识支撑。  相似文献   

镇江圌山绍隆禅寺“活地”成因     

蒋明镜  刘静德  肖俞  胡海军  武晓光  汤菲 《山地学报》2012,(1):93-98

"活地"是宗教的传奇,而由于以往知识与技术的限制以及宗教圣地的"不可侵犯性","活地"也成了大自然的千年未解之谜。通过现场考察和资料调研,明晰了"活地"所在地区的地质构造特征。采用高频率表面波监测、分析技术,通过现场试验,研究了"活地"附近地表浅层岩土体分布情况。采用图像分析技术,经室内试验研究得出了"活地"及周围地区出露岩石的矿物组成。最终,对于"活地"的成因提出以下看法:1.否定了地下深层生长性岩脉诱发"活地"现象的观点;2.膨胀岩及膨胀土吸水膨胀对"活地"的隆升有一定作用,但这不是"活地"的主要诱因;3.提出"活地"是岩石风化作用及特殊地理环境综合作用结果的观点:风化作用使岩体疏松、体积增大,地面隆起;两侧山体运动对其交界处岩石产生挤压作用,为"活地"的持续隆升提供动力源。  相似文献   

Detection of non-radial pulsation and faint companion in the symbiotic star CH Cyg     

E. Pedretti †  J. D. Monnier  S. Lacour  W. A. Traub  W. C. Danchi  P. G. Tuthill  N. D. Thureau  R. Millan-Gabet  J.-P. Berger  M. G. Lacasse  P. A. Schuller  F. P. Schloerb  N. P. Carleton 《Monthly notices of the Royal Astronomical Society》2009,397(1):325-334

We have detected asymmetry in the symbiotic star CH Cyg through the measurement of precision closure phase with the Integrated Optics Near-Infrared Camera (IONIC) beam combiner, at the infrared optical telescope array interferometer. The position of the asymmetry changes with time and is correlated with the phase of the 2.1-year period found in the radial velocity measurements for this star. We can model the time-dependent asymmetry either as the orbit of a low-mass companion around the M giant or as an asymmetric, 20 per cent change in brightness across the M giant. We do not detect a change in the size of the star during a 3-year monitoring period neither with respect to time nor with respect to wavelength. We find a spherical dust shell with an emission size of 2.2 ± 0.1 D _* full width at half-maximum around the M giant star. The star to dust flux ratio is estimated to be 11.63 ± 0.3. While the most likely explanation for the 20 per cent change in brightness is non-radial pulsation, we argue that a low-mass companion in close orbit could be the physical cause of the pulsation. The combined effect of pulsation and low-mass companion could explain the behaviour revealed by the radial velocity curves and the time-dependent asymmetry detected in the closure-phase data. If CH Cyg is a typical long secondary period variable then these variations could be explained by the effect of an orbiting low-mass companion on the primary star.  相似文献   

X-ray absorption contrast images of binary chemical reactions     

D. Walker  O.T. Lord  M.J. Walter  S.M. Clark   《Chemical Geology》2009,260(3-4):211-220

Low-divergence synchrotron-sourced X-rays enable a radiographic imaging scheme for full characterization of binary chemical reactions and characterization by type of more complex reactions, in situ, in diamond anvil cells (DAC). Spatially resolved reactants are induced to react by laser heating of their interface. The spatially intermediate products are observed through X-ray absorption contrast. Limits to the technique include the ability to maintain controlled experiment geometry during compression and the ability to resolve chemical differences between reactants and products by X-ray absorption. The ability to make in situ observations at experimental pressure and temperature obviates the problem with quenching techniques for capturing liquid compositions in experiments with dimensions smaller than the diffusion length during quenching time. Partially molten Fe-alloy systems, of poor quenchability, are examined at DAC pressures and temperatures for relevance to Earth's core constitution and evolution. Determinations of eutectic melting in Fe–FeS match known results. Of the probable light elements that may alloy with Fe in the Earth's liquid outer core, Fe–FeS experiments show only modest quenching problems, but C and Si alloy experiments are highly vulnerable to quenching artifacts. The observed reactivity of FeS, Fe₃C, FeSi, and FeO(OH) with Fe in DAC makes the observed non-reactivity between Fe and FeO more significant, reducing the probability that oxygen alone is the major alloy in Earth's molten outer core.  相似文献   

Converted phases analysis of the Campi Flegrei caldera using active seismic data     

T.M. Blacic  D. Latorre  J. Virieux  M. Vassallo   《Tectonophysics》2009,470(3-4):243-256

We applied a type of depth migration for converted seismic phases to active and passive seismic data sets from the Campi Flegrei volcanic region in southern Italy. The migration method is based on the diffraction summation migration technique. Travel times to grid points in a volume were calculated in smooth P and S-velocity models and trace energy near the calculated converted phase time was stacked over multiple sources at one receiver. Weighting factors based on Snell's Law at an arbitrarily oriented local interface were applied to better focus trace energy. PP reflection images from the active data set provide increased detail to images of the caldera rim from other studies. The migrated images also show features near 2–3 km in depth beneath Pozzuoli City, which may be associated with an over-pressured gas volume, as suggested by other geophysical investigations. Possible deeper features near 4 km depth may be related to the presence of the carbonate basement or may image a previously undetected feature, such as a small body of strongly thermometamorphosed volcanic rock. The current passive earthquake data set from the 1984 ground uplift episode was not well suited to the converted phases analysis due to narrow P–S windows and high noise levels in the traces. However, two stations provide confirmation and extension of imaged features in the active data.  相似文献   

地-空瞬变电磁法电阻率成像研究与应用   总被引：1，自引：0，他引：1  

马振军  底青云  薛国强  高雅 《地球物理学报》2021,64(3):1090-1105

地-空瞬变电磁法(Semi-airborne transient electromagnetic,SATEM)凭借适应能力强、探测深度大、实时性强等特点,适用于湖泊、沼泽、山区等地形复杂地区观测.SATEM接收数据量大、精度要求高,传统成像方法基于地面视电阻率计算未考虑飞行高度,开展SATEM的高精度快速成像研究对实际运用有重要作用.针对SATEM中电性源发射装置感应电流分布,接收装置设置于空中以及两者不在相同平面的特点,本文考虑横向、纵向感应电流差异,飞行高度对视电阻率影响等因素,提出电性源SATEM电阻率成像方法.首先,基于电性源瞬变电磁场感应电流分布特征及各分量空间分布、扩散特性分析,推导出基于均匀半空间磁场与感应电压解析解,然后定义了电性源地-空瞬变电磁法早期、晚期、全期视电阻率;最后根据对感应电流分布分析定义了横向分量和纵向分量的成像深度,并研究了成像深度受飞行高度、发射磁矩、偏移距、偏移角度的影响;对煤炭采空区的实测结果表明,利用本文提出的电阻率成像方法可以更加精确定位目标体位置.  相似文献   

利用区域辐射特性优化获取光学遥感数据     

冉琼  迟耀斌  吴双  文强 《遥感学报》2013,17(1):138-150

通过分析成像过程及其影响因素,提出了对成像积分时间进行控制的优化成像方法。首先建立成像参数模型,探讨了模型参数计算、成像过程中模型参数的选择,分析了图像后处理问题,并利用北京一号小卫星进行了遥感数据优化获取实验。实验结果表明,根据地物特性进行成像参数优化后获取的图像具有更宽的动态范围和更高的辐射分辨率,信息量和信噪比也大幅增强。  相似文献   

珠江口盆地惠州地区珠江组砂体上倾尖灭的地质-地球物理“逐级预测”方法     

芮志锋  林畅松  郭佳  杜家元  丁琳  李潇 《现代地质》2019,33(6):1229-1240

砂体上倾尖灭油气藏是岩性油气藏中重要类型之一,砂体上倾尖灭的刻画与描述是上倾尖灭圈闭有效性评价的关键。在以三角洲前缘沉积为主构成的三级层序内,三角洲沉积相关砂体上倾尖灭的地质-地球物理“逐级预测”描述方法对于认识上倾尖灭油气藏分布规律及其油气勘探具有重要意义。该方法由5个部分组成:在三级层序识别的基础上,运用高精度层序地层划分技术建立了四级层序构成的高频层序地层格架;在高频层序约束下,利用地震沉积学技术描述沉积相的平面分布;在地质模型指导下,利用频谱成像技术定性确定尖灭带的分布;利用相控储层反演半定量、定量预测砂体尖灭线;根据不同成因砂体的沉积特点,利用正演模拟技术开展尖灭线的外推预测。  相似文献   

多信息多技术深度速度建模技术在复杂构造中的应用研究     

赵玲芝  金守利  王成祥  曾庆芹 《物探化探计算技术》2019,(3):419-425

中国西部等复杂区的油气勘探潜力较大,但地质条件复杂,造成常规偏移成像的精度不够,给解释带来了诸多困难。根据其地质特点,围绕高精度成像的需求,开展高精度速度建模技术研究,形成了配套的技术策略,为其进一步改善复杂区的成像精度,落实勘探目标奠定了基础。在该配套技术中:基于真地表的速度建模技术可以通过真地表数据准备来解决现有大圆滑偏移基准面对成像波场的改变、初至层析近地表建模技术的应用弥补了反射建模技术在近地表应用的不足、多信息约束速度建模可提高速度模型的可靠性、各向异性假设的成像技术更加接近复杂构造地下介质的假设,这些技术的配套应用可以有效提高复杂区成像位置的精度和准确度。在实际资料中的应用充分说明该技术的有效性。  相似文献