地幔流体的前缘研究

地幔流体是与地幔环境处于平衡的气体和挥发分。其主要化学组分为碳、氢、氧、氮、硫（ＣＨＯＮＳ）。它以富于地球内部原始组分为特征，但也包含部分再循环组分。地幔挥发分在弱还原条件下主要为ＣＯ２－Ｈ２Ｏ，强还原环境则以ＣＨ４－Ｈ２Ｏ－Ｈ２为主。地幔流体地球化学的重要性质为：（１）易溶于硅酸盐熔体；（２）净化作用；（３）再沉淀作用。近年来，有关地幔流体中稀有气体和挥发分的起源、分布及同位素组成等前缘领域的研究已取得重要进展。当前拟优先探索的问题包括气体裂化与金刚石成因，非生物成因地幔烃，地幔流体与成矿作用，以及地幔挥发分注入与地壳重熔等。     

南天山蛇绿混杂岩和中天山南缘糜棱岩的40Ar/39Ar年龄及其大地构造意义

 ⁴⁰Ar/³⁹Ar同位素年龄测定,获得南天山蛇绿混杂岩基质黑云母石英片岩单矿物黑云母的两个坪年龄分别为(370.0±4.8)Ma和(259.0±3.3)Ma;中天山南缘长英质糜棱岩单矿物黑云母的坪年龄为(250.5±7.9)Ma,二云母花岗岩单矿物白云母的坪年龄为(348.9±0.3)Ma。结合南天山古生代沉积特征和塔里木及伊犁-哈萨克斯坦板块古地磁数据的综合分析,提出南天山晚泥盆世至石炭纪早期完成向伊犁-哈萨克斯坦板块的B型俯冲,中-晚二叠世进行陆内A型俯冲造山的板块碰撞演化模式。     

柿竹园钨多金属矿床的Re-0s同位素等时线年龄研究

柿竹园钨多金属矿床产于千里山复式岩体与泥盆系碳酸盐岩的接触部位。其成矿时代以往都是用矿体附近的花岗岩体年龄来间接推断。我们最近采用辉钼矿的Re-Os等时线定年法直接测定了与千里山第一期花岗岩有关的夕卡岩型矿体的矿化年龄为151.0±3.5Ma。该年龄晚于第一期花岗岩,但早于第二期花岗岩,从而证实了钨多金属矿化在花岗岩系列的早期早阶段也可以成矿。该年龄与野外观察的地质情况十分吻合,而辉钼矿是热液矿床中的常见矿物,说明这种测年方法是一种研究热液矿床成矿时代及其成因的重要手段。     

陕西蓝田地区新第三纪地层划分的几点讨论

蓝田地区灞河组和蓝田组的时代归属是我国三趾马动物群分期的关键问题之一。通过与府谷老高川三趾马动物群的对比及古地磁测定，该区新第三纪地层可分为上新统静乐组（原蓝田组上部）、蓝田组（原蓝田组下部）和灞河组．蓝田组的地质时代可归保德期庙梁亚期，地质年龄约为距今５．３—５．０Ｍａ期间．灞河组的地质时代可与喇嘛沟动物群的对比，为保德早期或稍早．     

石源龙地区岩浆岩的稀土元素和同位素地球化学

本章系统研究石源龙地区流纹质熔结凝灰岩、粒状碎斑熔岩、英安岩、星村中细粒黑云母花岗岩的铷锶同位素地质年龄，并根据锶、氧同位素和稀土元素含量讨论其地质意义     

原生金矿成矿年龄测定研究

金成矿年龄和矿源同位素组成的准确测定，对金矿地质研究和找矿具有重要意义。本文根据３年多野外和室内工作的总结，获得了多个典型矿床的年龄和同位素测定结果：华北古陆北缘北侧槽区乌花敖包金矿测定为１３０—１２０Ｍａ的晚期造山作用成矿；南侧台区赛乌素金矿为２１１±１５Ｍａ的再循环古陆改造成矿；中段台区后沟一黄土梁金矿为２４３±７Ｍａ的古陆再造成矿；胶东焦家－乳山金矿为１２２．７±３．４Ｍａ和１２８±２３Ｍａ的燕山期成矿；华夏古陆八宝山金银矿为１４０±５Ｍａ的火山热液成矿。     

焦作矿区电法探测导,含水构造的效果

应用直流电法仪在井下进行了工作面巷道底板电测深和掘进头超前探测，查清了工作面底板水层的富水性和掘进头前头的地质构造及含水情况。目前，大部分探测结果已得到生产实践的证实。     

Accretion and exhumation at a Variscan active margin, recorded in the Saxothuringian flysch

The Saxothuringian flysch basin, on the north flank of the Central European Variscides, was fed and eventually overthrust by the northwestern, active margin of the Tepla-Barrandian terrane. Clast spectra, mineral composition and isotopic ages of detrital mica and zircon have been analyzed in order to constrain accretion and exhumation of rocks in the orogenic wedge. The earliest clastic sediments preserved are of early Famennian age (ca. 370?Ma). They are exposed immediately to the NW of the suture, and belong to the par-autochthon of the foreland. Besides ultramafic (?ophiolite) material, these rocks contain clasts derived from Early Paleozoic continental slope sediments, originally deposited at the NW margin of the Saxothuringian basin. These findings, together with the paleogeographic position of the Famennian clastics debris on the northwestern passive margin, indicate that the Saxothuringian narrow ocean had been closed by that time. Microprobe analyses of detrital hornblendes suggest derivation from the “Randamphibolit” unit, now present in the middle part of the Saxothuringian allochthon (Münchberg nappes). Detrital zircons of metamorphic rocks formed a little earlier (ca. 380?Ma) indicate rapid recycling at the tectonic front. The middle part of the flysch sequence (ca. early to middle Viséan), both in the par-autochthon and in the allochthon, contains abundant clasts of Paleozoic rocks derived from the northwestern slope and rise, together with debris of Cadomian basement, 500-Ma granitoids and 380?Ma (early Variscan) crystalline rocks. All of these source rocks were still available in the youngest part of the flysch (c. middle to late Viséan), but some clasts record, in addition, accretion of the northwestern shelf. Our findings permit deduction of minimum rates of tectonic shortening well in excess of 10–30?mm per year, and rates of exhumation of ca. 3?mm/a, and possibly more.     

Solar modulation of cosmogenic nuclide production over the last millennium: comparison between C and Be records

For about the last 30 years it has been recognized that the high frequency component of the tree rings ¹⁴C/¹²C record is dominated by the modulation of the cosmic ray flux by the solar wind. In particular, it has been demonstrated that the three most recent periods of low sunspot occurrence were characterized by high values of atmospheric ¹⁴C/¹²C. During the last millennium other periods of high ¹⁴C/¹²C values were observed but their solar origin is still debatable. In the present work we compare these fluctuations with an independent record of cosmogenic ¹⁰Be measured in ice from the South Pole to check the solar origin of the observed ¹⁴C/¹²C variations. In order to compare quantitatively the results obtained on ¹⁰Be and ¹⁴C, it is necessary to take into account the different behaviour of these two cosmogenic isotopes, and especially the damping effect of the carbon cycle in the case of ¹⁴C. As an input to a 12-box numerical model we used the relative fluctuations of the ¹⁰Be concentrations record measured in South Pole ice and converted it into a synthetic ¹⁴C record. We took into account the fact that ¹⁰Be modulation is enhanced in polar regions due to the orientation of the geomagnetic field. As expected, the fluctuations of the modelled ¹⁴C record are much smaller (a factor of 20) than those observed for the raw ¹⁰Be record. In addition, the variations are smoother and shifted in time by a few decades. The ¹⁰Be-based ¹⁴C variations closely resemble the ¹⁴C measurements obtained on tree rings (R = 0.81). In particular, it is easy to identify periods of maximal ¹⁴C/¹²C which correspond to solar activity minima centred at about 1060, 1320 (Wolf), 1500 (Spörer), 1690 (Maunder) and 1820 (Dalton) yr A.D. Cross-correlation calculations suggest that there is no significant lag between the ¹⁰Be-based ¹⁴C and the tree-ring ¹⁴C records. Our study strongly suggests the dominance of the solar modulation on the cosmonuclide production variations during the last millennium.     

杭州地区石笋稳定同位素古气候探索

用１４Ｃ测年技术和稳定同位素地球化学古温度方法，对浙江省临安瑞晶洞穴的石笋进行了１４Ｃ的测年和碳、氢、氧同位素测试，获得５～１万年间杭州地区古气候演化记录、该记录表明，在５～１万年间有三次较明显的周期性古温度变化，最高温度为１４．９℃，最低温度为６．６℃，最大温差为８℃左右，平均温差３～５℃。这段时期正处在大理冰期后期，但大理冰期并不是一个持续的低温阶段，它至少有３次温度波动。与我们获得的石笋同位素古温度相一致。另外，我们将５～１万年间杭州地区古气候变化与同期东南沿海的海平面变化进行了对比，在时间上也较为吻合，也就是温度上升、海平面也上升，温度下降、海平面也随之下降