A Comparison Between Near-Infrared And Visible Imaging Of The Inner Coma Of Comet Hale-Bopp At Perihelion

We present a comparison between images of comet C/1995 O1 (Hale-Bopp) obtained from 12 March to 9 May 1997, with two telescopes of the Observatorio del Teide (IAC, Tenerife, Spain) in visible (Johnson-V filter) and three near-infrared narrowband filters (Brγ (2.166 μm), CO (2.295 μm), and K_con (2.260 μm)). No significant differences are observed between the images in the three near-infrared bands suggesting that any CO emission is very weak, or produced by an extended flat source. We do not find evidence for the existence of an additional infrared component due to emission by warm dust, or to dust grains of diverse composition and/or size. Visible and infrared images of the same rotational phase look almost identical, supporting the view that the observed jets and shells are mainly dust structures. This revised version was published online in July 2006 with corrections to the Cover Date.     

The influence of deformation partitioning on dissolution and solution transfer in low-grade tectonic mélange

Abstract Dissolution of quartz and the recryst-allization and re-equilibration of phyllosilicates produce the dark anastomosing seams that dominate microstructures of tectonic melange which occur in a low-grade, imbricated and multiply deformed, mid-Palaeozoic, intracra-tonic fiysch sequence in northeastern Australia. Seams are composed of very closely spaced or coalesced cleavage lamellae, which are very thin layers of extremely fine-grained phyllosilicates. Cleavage seams enclose lenses of silt-stone or greywacke, which formerly occurred in continuous sedimentary layers, indicating extremely heterogeneous and disruptive deformation. Microphacoids enclosed by cleavage seams have subtle shape asymmetries analogous to those of porphyroclasts. Phyllosilicate-preferred orientations within microphacoids commonly lie at a low angle to enclosing seams, and asymmetric relationships occur within seams. The shape and fabric asymmetries appear to be constant, and are regarded as analgous to S and C planes. The number and extent of seams, the amount of dissolution they indicate, and the efficiency of deformation partitioning imply some enhancement of chemical activity and substantial silica loss from the system. This, in turn, suggests the passage of large amount of silica-undersaturated fluid, and melanges may be zones of high fluid flow. However, the microstructures and the disruptive nature of the fabrics may also reflect the influence of high bulk shear strains and suggest some relationship between the shearing component of deformation and the development of cleavages and foliations.     

Ion composition and solar wind interaction: Observations of comet C/1995 O1 (Hale-Bopp)

The extraordinary brightness of comet Hale-Bopp (C/1995 O1) offered the rare opportunity to investigate its ion tail by observations over a wide range of wavelengths. For the first time, ion emission lines could be detected in the radio domain, originating from H₃O⁺, HCO⁺ and CO⁺ ions. Observations in the extreme ultraviolet range showed O⁺ emissions. Optical imaging observations show a spectacular detail of structures in the ion tail. The combined measurements of the ion spatial distribution and dynamic provide a wealth of information which needs to be understood in terms of models of the comet-solar wind interaction and ion-neutral molecule reactions in the coma. This revised version was published online in July 2006 with corrections to the Cover Date.     

Towards biomarker analysis of hydrocarbons trapped in individual fluid inclusions: First extraction by ErYAG laser

Fluid inclusions act as sealed vessels containing information about the fluid environment in which the minerals precipitated, and until decrepitated, the chemical composition of the fluid inside the inclusion stays intact. In many cases fluid inclusions contain trapped hydrocarbons, which may provide useful information in paleontological, organic geochemical and astrobiological research since they act as containers of non-contaminated organic matter with a defined minimum age. Here we present a novel concept for extraction of fluid inclusions in preparation for application to extract single fluid inclusions. The method is based on the illumination of a sample with an ErYAG laser (). The wavelength of the laser is absorbed by water and organic material, and with the minerals encapsulating the inclusions transparent to the wavelength, the fluid will expand and the inclusion will decrepitate. The initial results of our study demonstrate that fluid inclusions can be extracted by the use of an ErYAG laser, and that organic biomarkers may survive the process, readily available for GC–MS analysis.     

Photometry and Imaging of Comet C/2000 Wm1 (Linear)

Earth, Moon, and Planets -     

Temporal and spatial variations of canopy temperature over a C3?C4 mixture grassland

This study discusses the photosynthetic pathway types involved in canopy temperature measurements on a mixed grassland consisting of C₃ and C₄ plants (dominant species in biomass were Solidago altissima (C₃), Miscanthus sinensis (C₄), and Imperata cylindrica (C₄)). In the wet conditions immediately after the rainy season, the mean canopy temperature for S. altissima was the lowest among the dominant species, mainly due to its leaf conductance being twice as large as the other two species. Despite using the same C₄ photosynthetic pathway, M. sinensis had a lower apparent canopy temperature than I. cylindrica due to a smaller proportion of sunlit elements in the field of view. In the dry conditions during late July, the mean canopy temperatures of the three dominant species were within 0·3 °C of one another. These results can be explained by poor water conditions for C₃ species (S. altissima). The simultaneous survey of vegetation and thermal imaging can help clarify characteristics of C₃ and C₄ canopy temperature over complicated grassland. Copyright © 2006 John Wiley & Sons, Ltd.     

MS 1512–cB58: A case study of star formation, metal enrichment and superwinds in Lyman break galaxies

Recent advances in instrumentation and observing techniques have made it possible to begin to study in detail the stellar populations and the interstellar media of galaxies at redshift z = 3, when the universe was still in its ‘teen years’. I illustrate recent progress in this field with the latest observations of the gravitationally lensed galaxy MS 1512- cB58. This revised version was published online in September 2006 with corrections to the Cover Date.     

基于VC+ +的圆锥投影正解和反解软件设计与实现

随着GIS的日益发展和广泛普及,地理坐标和平面坐标之间相互转换需求不断增加。因为GIS,尤其是大型GIS中的空间数据往往来源于多种信息源,而各种信息源地图所采用的投影往往并不一致,各种坐标之间的变换就成为所有GIS软件不可避免的问题。此软件基于Visual C 开发平台,实现了在圆锥投影中(等角、等距离和等面积)地理坐标和平面坐标之间的相互转换。     

TEQC单点定位的系统性偏差分析

TEQC是由UNAVCO Facility研制的GPS数据预处理软件,可进行单历元C/A码伪距单点定位的计算,获得各历元GPS接收机的WGS84坐标。利用TEQC对大量GPS观测数据的计算表明:TEQC软件的单点定位结果在东坐标和高程方向上带有明显的系统性偏差。作者研制的单点定位软件GPP,由于考虑了地球自转、对流层折射和电离层折射等误差对GPS定位的影响,因此单点定位的结果较为准确,而且对上述系统性偏差产生的原因进行了分析和探讨。