The complex refractive index of limestone particles: an extension to the FIR range for Mars applications     

V Orofino  A BlancoS Fonti  A.C MarraN Polimeno 《Planetary and Space Science》2002,50(9):839-847

  相似文献   

上地幔超高压流体的金刚石压砧实验研究     

胡书敏  张荣华  张雪彤 《地质学报》2006,80(10):1588-1597

地球深部流体主要是NaCl-H2O溶液,越到地球深部,它赋存的温度、压力越高,性质状态也不断变化,反之,亦然。当NaCl-H2O流体进入和脱离(上升过程)超临界状态时,其性质会发生截然不同的变化,影响着各种地质过程。使用金刚石压砧在高温高压下原位观测流体的实验,用谱学方法,结合同步辐射光源技术,成为定量化研究地球深部高温超高压流体的有效方法。作者使用同步辐射光源的红外谱研究了10GPa下的NaCl-H2O溶液;在地球化学动力学实验室研究了3GPa,650℃下的NaCl-H2O溶液红外谱,此测量方法可以提供温度压力和体积等数据,能研究其状态。NaCl-H2O溶液红外谱表明水分子主要振动谱受压力和温度影响是不同的。压力增加促使水分子主要振动谱向低波数变化。但是温度增加的效应相反。常温高压下水被压缩,结晶向紧密堆积变化。高温高压下的水有气、液、固和超临界流体各相。水分子间的氢键在近临界态开始减弱,氢键网络被破坏。  相似文献   

断层失稳错动热场前兆模式：雁列断层的实验研究   总被引：14，自引：4，他引：14       下载免费PDF全文

马瑾  刘力强  刘培洵  马胜利 《地球物理学报》2007,50(4):1141-1149

在实验室使用红外热像仪和接触式测温仪同步观测记录了压性和张性雁列断层失稳错动前后的热场变化过程.从实验记录中发现，在断层失稳引起温度场和热红外辐射亮温温度场上升之前，在两断层段之间的岩桥区发生降温变化.断层带开始升温发生在失稳前2～3 s内，岩桥区的降温却发生在失稳前约20s，这两个超前时间长度相差近一个量级.此类热场先降后升变化过程在雁列构造变形中有一定的普遍性，可能作为雁列断层失稳错动的热场前兆模式.根据实验观测结果，详细描述了上述热场变化的时间过程及其空间分布特征，分析了产生此种失稳前兆模式的机制，显著异常出现的条件及有利观测部位，讨论了它在地震前兆探索等研究中的意义.  相似文献   

Testing satellite and ground thermal imaging of low-temperature fumarolic fields: The dormant Nisyros Volcano (Greece)   总被引：1，自引：0，他引：1  

E. Lagios  S. Vassilopoulou  V. Sakkas  V. Dietrich  B.N. Damiata  A. Ganas 《ISPRS Journal of Photogrammetry and Remote Sensing》2007,62(6):447-460

The Nisyros Volcano (Greece) was monitored by satellite and ground thermal imaging during the period 2000–2002. Three night-scheduled Landsat-7 ETM⁺ thermal (band 6) images of Nisyros Island were processed to obtain land surface temperature. Ground temperature data were also collected during one of the satellite overpasses. Processed results involving orthorectification and 3-D atmospheric correction clearly show the existence of a thermal anomaly inside the Nisyros Caldera. This anomaly is associated mainly with the largest hydrothermal craters and has land surface temperatures 5–10 °C warmer than its surroundings. The ground temperature generally increased by about 4 °C inside the main crater over the period 2000–2002. Ground thermal images of the hydrothermal Stephanos Crater were also collected in 2002 using a portable thermal infrared camera. These images were calibrated to ground temperature data and orthorectified. A difference of about 0–2 °C was observed between the ground thermal images and the ground temperature data. The overall study demonstrates that satellite remote sensing of low-temperature fumarolic fields within calderas can provide a reliable long-term monitoring tool of dormant volcanoes that have the potential to reactivate. Similarly, a portable thermo-imager can easily be deployed for real-time monitoring using telemetric data transfer. The operational costs for both systems are relatively low for an early warning system.  相似文献   

莫来石陶瓷在电学和光学中的应用研究          下载免费PDF全文

靳正国  吕楠 《地质找矿论丛》1998,13(4):85-89

莫来石在电子,光学和高温结构中的应用已广泛以受到关注。本文介绍了以电子基板材料和红外辐射材料为应用背景下,有关莫来石基陶瓷的组成与性能间的关联研究,显示了新型莫来石材料在这些应用领域的潜在优良和良好的应用前景。  相似文献   

绿柱石中隧道水的红外光谱     

李湘祁  袁奎荣 《矿产与地质》1998,12(3):193-196

应用富时叶变换红外谱仪研究了三个启三绿柱石样（包括原样与热处理）。将３４３５ｃｍ＾－１宽吸收带归属于与铁离子成键的水。谱图表明隧道水的大量脱去是在８００℃以上的温度开始的,对于富碱样品,更可能是在１０００℃以后开始。隧道中碱金属离子的阻塞作用是造成绿柱石隧道水难以失去的重要原因．  相似文献   

Saturn's auroral/polar H₃ infrared emission: I. General morphology and ion velocity structure     

Tom Stallard  Steve Miller  Makenzie Lystrup  Nicholas Achilleos 《Icarus》2007,189(1):1-13

  相似文献   

Physical investigation of the potentially hazardous Asteroid (144898) 2004 VD17     

F. De Luise  D. Perna  E. Dotto  I.N. Belskaya  G.B. Valsecchi  A. Rossi  P. Paolicchi 《Icarus》2007,191(2):628-635

In this paper we present the observational campaign carried out at ESO NTT and VLT in April and May 2006 to investigate the nature and the structure of the near-Earth object (144898) 2004 VD17. In spite of a great quantity of dynamical information, according to which it will have a close approach with the Earth in the next century, the physical properties of this asteroid are largely unknown. We performed visible and near-infrared photometry and spectroscopy, as well as polarimetric observations. Polarimetric and spectroscopic data allowed us to classify 2004 VD17 as an E-type asteroid. A good agreement was also found with the spectrum of the aubrite meteorite Mayo Belwa. On the basis of the polarimetric albedo (pv=0.45) and of photometric data, we estimated a diameter of about 320 m and a rotational period of about 2 h. The analysis of the results obtained by our complete survey have shown that (144898) 2004 VD17 is a peculiar NEO, since it is close to the breakup limits for fast rotator asteroids, as defined by Pravec and Harris [Pravec, P., Harris, A.W., 2000. Icarus 148, 12-20]. These results suggest that a more robust structure must be expected, as a fractured monolith or a rubble pile in a “strength regime” [Holsapple, K.A., 2002. Speed limits of rubble pile asteroids: Even fast rotators can be rubble piles. In: Workshop on Scientific Requirements for Mitigation of Hazardous Comets and Asteroids, Washington, September, 2002].  相似文献   

Composition of hydrated near-Earth object (100085) 1992 UY4     

Eric L. Volquardsen  Andrew S. Rivkin 《Icarus》2007,187(2):464-468

Near-infrared spectra of the near-Earth object (100085) 1992 UY4 are similar to those of P-type asteroids, providing a fitted geometric albedo of 0.052±0.005 and an effective diameter of 1.68±0.08 km. This object, with a likely outer-belt origin, also exhibits a 3-μm absorption feature with a band depth of 3%±1%, corresponding to a regolithic bulk hydrogen-to-silicon ratio of 0.30±0.05. The bulk of this hydrogen seems to be present in H₂O-dominated minerals.  相似文献   

Evidence for enhanced hydration on the northern flank of Olympus Mons, Mars     

Giancarlo Bellucci  Joern Helbert  Francesca Altieri  Dennis Reiss  Jean-Pierre Bibring  Stephan van Gasselt  Harald Hoffmann  Yves Langevin  Gerhard Neukum  Franois Poulet 《Icarus》2007,192(2):361-377

In this paper we report about a small region on the northern scarp of Olympus Mons showing an increase of the 3 μm hydration band in the OMEGA spectra, together with low superficial temperatures. Although water ice clouds can occurs on the flank of big martian volcanoes, radiative transfer modeling indicates that atmospheric water ice alone cannot justify the shape of the observed band. A fit of the 1.9–3 μm absorption features is obtained by hypothesizing that the study region consists of a mixture of dust and water ice covered by an optically thin (τ=0.08 at 3 μm) layer of dust. Thermal modeling also suggests that water ice in this region may be stable during most of the martian year due to the saturation of the atmosphere. If water ice is responsible for the observed spectral behavior, it might consist of a number of ice or snow patches possibly deposited in small depressions.  相似文献