白垩纪温度较冷的估价

白垩纪温度较冷的估价Ｂ．ｗ．Ｓｅｌｌｗｏｏｄ等有关白垩纪气候的概念部分基于详尽的地质证据，如不耐寒冷的古生物（如：珊瑚的分布比现在偏极地５－１５℃）和特殊气候条件的沉积相的广泛分布。这些资料的解释反映２１℃的等温线在纬度上至少向两极移动５°，全球的平...     

Integrated chronostratigraphy of Proterozoic-Cambrian boundary beds in the western Anabar region, northern Siberia

Carbonate-rich sedimentary rocks of the western Anabar region, northern Siberia, preserve an exceptional record of evolutionary and biogeochemical events near the Proterozoic/Cambrian boundary. Sedimentologically, the boundary succession can be divided into three sequences representing successive episodes of late transgressive to early highstand deposition; four parasequences are recognized in the sequence corresponding lithostratigraphically to the Manykal Formation. Small shelly fossils are abundant and include many taxa that also occur in standard sections of southeastern Siberia. Despite this coincidence of faunal elements, biostratigraphic correlations between the two regions have been controversial because numerous species that first appear at or immediately above the basal Tommotian boundary in southeastern sections have first appearances scattered through more than thirty metres of section in the western Anabar. Carbon- and Sr-isotopic data on petrographically and geochemically screened samples collected at one- to two-metre intervals in a section along the Kotuikan River, favour correlation of the Staraya Reckha Formation and most of the overlying Manykai Formation with sub-Tommotian carbonates in southeastern Siberia. In contrast, isotopic data suggest that the uppermost Manykai Formation and the basal 26 m of the unconformably overlying Medvezhya Formation may have no equivalent in the southeast; they appear to provide a sedimentary and palaeontological record of an evolutionarily significant time interval represented in southeastern Siberia only by the sub-Tommotian unconformity. Correlations with radiometrically dated horizons in the Olenek and Kharaulakh regions of northern Siberia suggest that this interval lasted approximately three to six million years, during which essentially all 'basal Tommotian' small shelly fossils evolved.     

Origin of the hydrocarbon component of carbonaceous chondrites: the star-meteorite connection

We report the results of an experiment that produced a residue which closely matches the hydrocarbon component of the Murchison carbonaceous chondrite. This experiment suggests that the parent material of the meteoritic component originated as polycyclic aromatic hydrocarbon species in carbon stars during their later stages of evolution. The experiments also indicate that the pathway from those formation sites to eventual incorporation into the meteorite parent body involved hydrogenation in a plasma in the solar nebula or in H II regions prior to the solar nebula. This model is consistent with what is known about the meteoritic hydrocarbon component including deuterium abundance, the observation of cosmic infrared emission bands best attributed to polycyclic aromatic hydrocarbon molecules, and the inherent stability of these molecules that allows their formation in stars and subsequent survival in the interstellar medium.     

丘陵草坡土壤10Be分布特征及土壤生成速率

以位于广东省境内的中国科学院鹤山丘陵综合试验站草坡集水区土壤剖面为对象, 对土壤样品进行了大气成因¹⁰Be测定, 对基岩以及风化岩石样品进行了就地(in-situ)宇宙成因¹⁰Be测定. 基于土壤层大气成因¹⁰Be测定, 参考土壤层底界¹⁴C表观年龄, 估算出草坡地区3800年以来大约有34%的成土物质被侵蚀掉; 基于风化岩石间隙土大气成因¹⁰Be测定, 估算得到基岩之上90 cm厚的风化岩石层至少经历了1.36 Ma, 平均侵蚀速率约为1.26×10^-4 cm/a. 表面风化岩石和基岩就地成因¹⁰Be浓度分别为10.7×10⁴ atoms/g和 8.31×10⁴ atoms/g, 据此估算得到: 土壤生成速率为8.8×10^-4 cm/a; 表层风化岩石以及基岩宇宙射线暴露时间分别约为7.2×10⁴和2.3×10⁵a. 土壤生成速率大于侵蚀速率, 自然地貌状况稳定.     

斐济一汤加地幔过渡带的地震波各向异性

论述了一个不常见的、明显的过渡带(TZ)各向异性的实例，证据来自于许多比垂直偏振剪切波(SV)早到3S的水平偏振剪切波(SH)。各向异性区与远离活动俯冲带及已知的纵、横波速度横向非均匀体边界的深震相关。我们把这一各向异性区解释为与岩石层残骸中的巨大岩石异常体有关的强组构，这个巨大的岩石异常体悬浮并滞留于过渡带中。冷板块的快速俯冲非常适合于这种组构的形成，因此板块穿透到下地幔并不能普遍发生。     

利用地理挖掘概念推动地理知识获取的可行性研究:第一篇

总结了近阶段一系列的多媒体用于检索各种为空间信息提供图形接口的方式。在20世纪 80年代这种方法导致产生了交互式的原型激光碟,用于评价媒体在信息发布上的有效性,随后提出并发展了地理挖掘概念。地理挖掘概念是     

The Preliminary Statistical Analysis of LAMOST DR8 Low Resolution AFGK Stars

We download the Large sky Area Multi-Object fiber Spectroscopic Telescope Data Release 8(LAMOST DR8)low resolution catalog for 6,478,063 AFGK type stars and plot the figures of effective temperature,gravitational acceleration and metal abundance.Some small and medium mass stars are evolved from pre-main sequence or main sequence stage to planetary nebula stage or white dwarf stage by the stellar evolution code MESA.We analyze the observed statistical data and model calculation results,and then o...