Regional Geochemical Division—A Tool for Delineating Geochemical Block

INTRODUCTIONGeochemists need to study the spatial distribution of theassociations of the geochemical elements(AGE) to delineatethe geochemical blocks or recognize geochemical anomalies inregional geochemical exploration.Regional geochemical divi-sion (RGD) is a mapping technique for the division of thestudy area into slices where the natural AGEs are relativelysimple and uniform.A practical approach to RGD is to digital-ly devide the collected geochemical samples into groups bymeans o…     

GEOLOGICAL STUDIES OF METAMORPHIC ROCKS IN THE VICINITY OF M.C.T./LESSER HIMALAYAN SHEAR ZONE, PARTS OF SIKKIM HIMALAYAS

GEOLOGICAL STUDIES OF METAMORPHIC ROCKS IN THE VICINITY OF M.C.T./LESSER HIMALAYAN SHEAR ZONE, PARTS OF SIKKIM HIMALAYAS     

PERSISTENCES IN THE δ~(13)C AND δ~(18)O FROM TS95, A LAKE CORE AT THE SOUTH FRANK OF WEST KUNLUN MOUNTAIN

PERSISTENCES IN THE δ~(13)C AND δ~(18)O FROM TS95, A LAKE CORE AT THE SOUTH FRANK OF WEST KUNLUN MOUNTAIN     

Orbit of comet C/1860 M1 (Great Comet of 1860)

Comet C/1860 M1 (Great Comet of 1860) is one of a large number of comets with parabolic orbits. Given that there are sufficient observations of the comet, 261 in right ascension and 251 in declination, it proves possible to calculate a better orbit. The comet's orbit is hyperbolic, and statistically different from a parabola. The comet, therefore, cannot be considered to be a Near Earth Oject. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

罗兰-C最新进展及其对我国相关系统改造的启示

介绍了罗兰－Ｃ的最新进展。风险评估表明基系统（ＧＰＳ、ＧＬＯＮＡＳＳ）不能作为唯一的导航、定位、定时手段。现代罗兰－Ｃ系统的性能已得到较大改善,也具有发播关分ＧＰＳ、ＤＧＬＯＮＡＳＳ等数据的通信能力。它与星基系统能以多种方式组合,可以获得比单独一个系统更好的民航、定位、授时性能。最后讨论了我国相关系统发展的一些体会和设想。     

离石丰义剖面2.50 MaB.P.前后地质事件研究

对离石丰义剖面红土与黄土之间发育的厚约２ｍ的岩性混杂层从磁性地层、稳定同位素、天体撞击事件等方面进行了分析与探讨,初步认为Ｍ／Ｇａ界限位于岩性混杂层中部,从Ｎ２红土到岩性混杂层,气候由干热暖湿转变;由岩性混杂层到第四纪黄土,气候由暖湿向干冷转化 ;在岩性混杂层中发现有蛎量的强磁性微颗粒,可能为微玻璃陨石或铁质陨石,这可能意味着一次天体撞击事件的发生。     

类星体3C 286的一个早期VLBI观测结果

利用基于自校正和ＣＬＥＡＮ算法的现代ＶＬＢＩ混合成图技术,对Ｐｅａｒｓｏｎ等人于１９７６年观测得到的类星体 ３Ｃ ２８６在 １８ ｃｍ波段上的 ＶＬＢＩ数据重新作了处理．由此得到的图像要大大好于最初的处理结果,也获得了更多的有用信息．用几个Ｇａｕｓｓ模型去拟合校正后的ＵＶ数据,发现中央亮区可以被分解为两个致密结构,这与后来的高分辨率观测相一致．与不同历元的ＶＬＢＩ观测结果相比较,发现这两个致密结构间的距离不但在同一时间随观测频率变化,而且很有可能在同一观测频率上随时间变化．     

相邻四片Bezier曲面的C1连续光滑拼接

相邻的多片 Bezier曲面拼接时 ,在边界处容易引起连续性问题。作者提出了一种方法 ,通过构造逼近曲面片 ,在相邻的四片曲面片边界及交点处达到 C1连续。该方法的关键点在于确定交点周围曲面片上相互关联的四个 Bezier控制点 ,使得曲面片在交点处达到 C1连续 ,并给出了逼近曲面片与原曲面片误差比较公式及误差估计方法     

The infrared jet in 3C 66B

We present images of infrared (IR) emission from the radio jet in 3C 66B. Data at three wavelengths (4.5, 6.75 and 14.5 μm) were obtained using the Infrared Space Observatory . The 6.75-μm image clearly shows an extension aligned with the radio structure. The jet was also detected in the 14.5-μm image, but not at 4.5 μm. The radio–infrared–optical spectrum of the jet can be interpreted as synchrotron emission from a population of electrons with a high-energy break of 4×10¹¹ eV. We place upper limits on the IR flux from the radio counter-jet. A symmetrical, relativistically beamed twin-jet structure is consistent with our results if the jets consist of multiple components.     

柴达木盆地东部表土花粉分析

柴达木盆地东部荒漠区 8个样地、 2 3个样点的表土花粉分析较好地揭示了荒漠区花粉组合的特点及其与植被、环境的关系。研究发现 ,荒漠区表土花粉以藜科 (Chenopodiaceae)和蒿属 (Artemisia)为主 ,并以前者占优势地位 ,麻黄属 (Ephedra)亦较常见 ,禾本科(Gramineae)、菊科 (Compositae)植物在群落中也占有一定的比例。花粉百分比含量DCA排序与相关分析发现 ,荒漠区不同植物群落下表土花粉组合特征各不相同 ,而且与相应的植物群落及其所代表的环境特征相一致。荒漠区表土花粉蒿 /藜 (Artemisia/Chenopodiaceae)比对干旱程度具有指示作用 ,比值越小 ,越干旱。