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????JPL DE?????????洢??????????????????????????????????DE??????????????????????????20???DE406?????????????369 kb????????1/6????GPS??????????ü???DE????????????????????飬?????????60?????????????????????3 m???ü??????????????????????????????????????????????С?????????洢??????????????????????Ч???     

眼眶肌锥内血管外皮细胞瘤的CT及MRI诊断

目的:探讨眼眶肌锥内血管外皮细胞瘤(HPC)的CT及MRI表现和病理组织学特点,旨在提高对HPC的认识。方法:结合文献复习,回顾性分析1例经手术病理证实的HPC影像学表现、病理组织学特点、治疗及预后。结果:HPC的CT表现为眼眶内软组织密度;MRI表现以等T1信号、长T2信号为主,内见特征性多发细小流空信号,眼内肌及视神经明显受压,球后脂肪间隙存在。增强扫描:病变呈不均匀强化。结论:深入了解HPC的CT及MRI表现和病理组织学特点,对HPC的诊断、治疗和预后具有重要价值。      

Improved-GRACE����������������Ż��о�

???????????????????ü????????????????GPS????????λ????????????????????????????????????????????????????????????????Improved??GRACE?????????????????????????????????????????????1????300?????????350 km???????????????????????3.993??10 ^-1 m??????300 km??250 km???????????????????8.770????77.145????????400 km??450 km??????????????????8.718????75.307????2??????50 km???????????????????????3.993??10^-1 m??????110 km??220 km??????????????????1.259????1.395????3????????????Improved??GRACE????????????????????????????????350 km??50 km?????     

最近11万年来东亚季风轨道与千年尺度气候变率在南京下蜀黄土中的记录

对南京李家岗下蜀黄土剖面上部的近20 m地层进行野外观察和室内研究,划分出5层黄土和5层古土壤,按5 cm间距采集了Rb/Sr、色度、磁化率和粒度样品,并在剖面和可追索的相邻剖面上采集了13个光释光测年样品。分析结果显示,Rb/Sr、色度和磁化率等夏季风代用指标曲线所表现的4次岁差变率振荡具有高度的一致性,依据气候地层...     

柴达木盆地自然伽玛曲线记录的古气候变化对太阳辐射响应关系的对比研究

采用柴达木盆地达参1井自然伽玛(GR)曲线,建立了2 85MaBP以来的轨道调谐时标.对GR曲线、深海记录和黄土记录与太阳辐射曲线时频域的多维谱分析及奇异谱分析结果表明:达参1井GR曲线相对于太阳辐射的滞后时间短于深海及黄土记录3～4ka,GR曲线记录的岁差周期成分更为显著,且与太阳辐射在岁差周期上显示了更强的相关性.表明盆地古气候演化受到太阳辐射岁差周期强烈影响,具有低纬陆地记录的特征,而与深海记录和黄土记录受轨道倾斜周期和全球冰量变化的重要影响有别.     

Drivers of ecosystem and climate change in tropical West Africa over the past ∼540 000 years

A paucity of empirical non‐marine data means that uncertainty surrounds the impact of climate change on terrestrial ecosystems in tropical regions beyond the last glacial period. The sedimentary fill of the Bosumtwi impact crater (Ghana) provides the longest continuous Quaternary terrestrial archive of environmental change in West Africa, spanning the last ～1.08 million years. Here we explore the drivers of change in ecosystem and climate in tropical West Africa for the past ～540 000 years using pollen analysis and the nitrogen isotope composition of bulk organic matter preserved in sediments from Lake Bosumtwi. Variations in grass pollen abundance (0?99%) indicate transitions between grassland and forest. Coeval variations in the nitrogen isotopic composition of organic matter indicate that intervals of grassland expansion coincided with minimum lake levels and low regional moisture availability. The observed changes responded to orbitally paced global climate variations on both glacial–interglacial and shorter timescales. Importantly, the magnitude of ecosystem change revealed by our data exceeds that previously determined from marine records, demonstrating for the first time the high sensitivity of tropical lowland ecosystems to Quaternary climate change.

     

成矿元素富集机制的量子地球化学研究——以攀枝花钒钛磁铁矿矿床为例

攀枝花钒钛磁铁矿矿床为富集钒、钛、铁等过渡元素的典型岩浆矿床。文章运用量子地球化学的理论和方法研究该矿床的元素组合、分配及变化特征 ,并用量子力学理论的abini tioHartree Fock分子轨道法对钛磁铁矿和钛铁矿晶体结构进行了模拟计算。结果表明 :源于地幔的原始岩浆富集成矿元素 ;在其结晶过程中 ,V ,Ti,Fe等成矿元素再次富集于钛磁铁矿和钛铁矿中而形成矿床 ,这种再富集受晶体结构择位能控制。     

地球轨道偏心率变化对东亚季风气候模拟的影响

采用较为真实的椭圆轨道代替了原区域气候模式中的圆近似轨道,并进行了10年模拟试验,用以了解该模式对东亚季风区气候年际变化的模拟能力,同时比较地球轨道参数计算变化对现代东亚季风气候模拟的影响.结果表明:当把模式中的地球轨道计算从圆形改为椭圆时,中国东部的降水模拟有所改进,东亚地区的温度、降水、比湿等气候要素均出现夏季降低(减少)而冬季升高(增加)的季节变化趋势,而且亚洲冬、夏季风也均有减弱.但从总体上说,现代气候状况的模拟对地球公转轨道的计算方案不敏感.通过该工作的模拟研究说明,对较短时期的现代气候模拟,地球公转轨道采用圆近似是可行的.     

地球公转轨道偏心率变化的构造运动响应

最近3Ma发生的主要构造运动和气候变化事件,在准0.4Ma周期上与地球轨道偏心率变化存在一致性。据黄土高原地层记录划分的构造气候旋回界限,日历年龄分别为0.07、0.46、0.83、1.32、1.70、2.08、2.74MaBP,对应于偏心率曲线波动幅度由大变小时段的特定转折位置。文中分析了地球公转运动变速的基本数据及其对地球自转运动和圈层相互作用的可能影响,探讨了轨道偏心率变化对构造运动的驱动机制,并指出了构造气候旋回研究可为地质力学理论发展展示良好的前景。      

Orbital dispersion of comet Encke's meteoroids

The orbital evolution of model meteoroids ejected from the comet Encke has been investigated. The particles abandon the mother body with velocities 20 and 40 ms^-1 perihelion within the interval of the past 10,000 years. Their 10,000 years old osculating orbits were numerically integrated forward, using a dynamical model of the solar system consisting of all planets. Forces from solar electromagnetic and corpuscular radiation effecting the particles are considered, too. Orbital dispersions of the model meteoroids are presented. The importance of nongravitational forces for a long-term orbital evolution of meteoroid streams is shown.