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31.
We discuss wind variability in intermediate luminosity B supergiants. Because these are not the hottest, most luminous or just about other kind of -est stars, they have not attracted much attention. However, since their wind lines are well-developed, but unsaturated, they make ideal diagnostics for time dependent wind studies. We show that their wind profiles undergo large scale variability and that this phenomenon is quite common. We also discuss a time series for the B0.5 Ib HD 64760 which suggests the long sought after connection between wind and photospheric activity. Newly developed analysis techniques needed to extract physical information from the wind lines are discussed, and results are applied to the time series.  相似文献   
32.
松潘- 甘孜造山带巨厚的三叠系复理石沉积盖层给探讨其基底性质、俯冲- 碰撞过程和深部岩浆作用增添了难度,使得带内广泛出露的花岗质岩体和少量镁铁质岩体成为解开松潘- 甘孜造山带构造演化谜团的重要研究对象。锆石U- Pb定年结果表明道孚花岗闪长岩形成于223. 5~217. 4 Ma,炉霍二长岩结晶年龄为219. 4 Ma,辉长岩为218. 9 Ma,均属于晚三叠世岩浆活动的产物。化学成分研究结果表明,花岗质岩石都表现出I型花岗岩特征,其中炉霍二长岩具有较高的Ba、Sr含量,相对较高且均一的εHf(t)值(-3. 69~-1. 65),表明其可能来源于富集玄武质新生下地壳的熔融。道孚花岗闪长岩具有分散的εHf(t)值(-13. 51~0. 41),野外和地球化学特征指示其形成于幔源熔体与古老壳源熔体的混合。辉长岩在微量元素蜘蛛图上具有类似的模式,不同程度富集Ba、Sr、Pb、Th和U元素,出现Nb、Ta、Ti元素亏损,具有岛弧玄武岩的特征,来源于流/熔体交代的地幔楔部分熔融。综合区域已有资料,我们对甘孜- 理塘洋的演化历史提出新的认识,认为甘孜- 理塘洋不仅仅存在向南俯冲的可能性,同时也具有北向俯冲的历史,晚三叠世道孚- 炉霍岩浆岩的形成受控于甘孜- 理塘洋向北边松潘- 甘孜地块俯冲的背景之下。  相似文献   
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Garnets in continentally derived high-pressure (HP) rocks ofthe Sesia Zone (Western Alps) exhibit three different chemicalzonation patterns, depending on sample locality. Comparisonof observed garnet zonation patterns with thermodynamicallymodelled patterns shows that the different patterns are causedby differences in the water content of the subducted protolithsduring prograde metamorphism. Zonation patterns of garnets inwater-saturated host rocks show typical prograde chemical zonationswith steadily increasing pyrope content and increasing XMg,together with bell-shaped spessartine patterns. In contrast,garnets in water-undersaturated rocks have more complex zonationpatterns with a characteristic decrease in pyrope and XMg betweencore and inner rim. In some cases, garnets show an abrupt compositionalchange in core-to-rim profiles, possibly due to water-undersaturationprior to HP metamorphism. Garnets from both water-saturatedand water-undersaturated rocks show signs of intervening growthinterruptions and core resorption. This growth interruptionresults from bulk-rock depletion caused by fractional garnetcrystallization. The water content during burial influences significantly thephysical properties of the subducted rocks. Due to enhancedgarnet crystallization, water-undersaturated rocks, i.e. thoselacking a free fluid phase, become denser than their water-saturatedequivalents, facilitating the subduction of continental material.Although water-bearing phases such as phengite and epidote arestable up to eclogite-facies conditions in these rocks, dehydrationreactions during subduction are lacking in water-undersaturatedrocks up to the transition to the eclogite facies, due to thethermodynamic stability of such hydrous phases at high P–Tconditions. Our calculations show that garnet zonation patternsstrongly depend on the mineral parageneses stable during garnetgrowth and that certain co-genetic mineral assemblages causedistinct garnet zonation patterns. This observation enablesinterpretation of complex garnet growth zonation patterns interms of garnet-forming reactions and water content during HPmetamorphism, as well determination of detailed P–T paths. KEY WORDS: dehydration; high-pressure metamorphism; Sesia Zone; subduction; thermodynamic modelling  相似文献   
37.
Two apparently distinct, sub-parallel, paleo-subduction zonescan be recognized along the northern margin of the Tibetan Plateau:the North Qilian Suture Zone (oceanic-type) with ophioliticmélanges and high-pressure eclogites and blueschistsin the north, and the North Qaidam Belt (continental-type) inthe south, an ultrahigh-pressure (UHP) metamorphic terrane comprisingpelitic and granitic gneisses, eclogites and garnet peridotites.Eclogites from both belts have protoliths broadly similar tomid-ocean ridge basalts (MORB) or oceanic island basalts (OIB)in composition with overlapping metamorphic ages (480–440Ma, with weighted mean ages of 464 ± 6 Ma for North Qilianand 457 ± 7 Ma for North Qaidam), determined by zirconU–Pb sensitive high-resolution ion microprobe dating.Coesite-bearing zircon grains in pelitic gneisses from the NorthQaidam UHP Belt yield a peak metamorphic age of 423 ±6 Ma, 40 Myr younger than the age of eclogite formation, anda retrograde age of 403 ± 9 Ma. These data, combinedwith regional relationships, allow us to infer that these twoparallel belts may represent an evolutionary sequence from oceanicsubduction to continental collision, and continental underthrusting,to final exhumation. The Qilian–Qaidam Craton was probablya fragment of the Rodinia supercontinent with a passive marginand extended oceanic lithosphere in the north, which was subductedbeneath the North China Craton to depths >100 km at c. 423Ma and exhumed at c. 403 Ma (zircon rim ages in pelitic gneiss). KEY WORDS: HP and UHP rocks; subduction belts; zircon SHRIMP ages; Northern Tibetan Plateau  相似文献   
38.
刘辰生  郭建华  苏娟 《新疆地质》2005,23(3):288-291
阿克库勒地区卡拉沙依组碎屑岩储层的成分成熟度和结构成熟度均较低.储层的次生溶蚀孔隙所占比例远高了:原生孔隙,次生孔隙是储层的主要储集空间.样品数据统计显示,卡拉沙依组储层属于低孔、低渗储层类型.根据岩石薄片、铸体薄片观察及储层样品的扫描电镜和阴极发光分析结果,本区石炭系储层主要经历的成岩作用有压实(压溶)作用、胶结作用、溶蚀作用和交代作用,其中碳酸盐矿物的沉淀和溶蚀作用是本区卡拉沙依组储层所经历的最重要的成岩作用.成岩作用已达到晚成岩B期,早期方解石交代石英颗粒并发生大量溶蚀,生成大量次生孔隙,晚期方解石没有发生溶蚀.  相似文献   
39.
苏鲁造山带超高压变质作用及其P-T-t轨迹   总被引:23,自引:25,他引:23  
基于超高压变质岩的岩石学,特别是超高压矿物生长成分环带、扩散环带和蚀变作用研究,综合前人的岩石学和年代学研究成果,提出苏鲁造山带超高压变质作用峰期发生在1000-1100℃和6-7GPa条件下,俯冲深度相当于200km,形成年代为240-250Ma。在此基础上,重塑了一个包括八期变质作用的P-T-t轨迹,揭示出超高压变质岩经历了三个不同的折返阶段,即从200km到100km深度的快速折返阶段,抬升速率为5km/Ma,冷却速率为10℃/Ma;从100km到30km的快速折返,抬升速率为4km/Ma,或为近等温降压,或为缓慢降温的快速降压过程;从下地壳到近地表的缓慢折返阶段,抬升速率为1km/Ma,但为快速降温过程,冷却速率可达20℃/Ma。  相似文献   
40.
错卧莫-惩香错火山-沉积盆地位于西藏冈底斯陆块中部南缘。盆地内火山-沉积地层称古新世-渐新世林子宗群,岩石地球化学数据分析表明:这套火山岩系属钙碱性系列,轻稀土富集,不同程度表现出负Eu、负Ce、负Nb异常。微量元素K、Rb、Th、Ce富集,Sr、Ba,尤其是Nb、P、Ti亏损。初步认为这套火山-沉积岩系形成于俯冲造弧的构造背景中,是来自于俯冲带的地幔源区基性分异岩浆与陆壳重熔的酸性岩浆在不同的时间段内,按不同的比例混合形成的。同时,俯冲板块上深海沉积物与基性岩浆混合作用也是不容忽视的因素。在综合分析基础上,笔者认为印度板块与欧亚板块的碰撞启动时间在45Ma以后。  相似文献   
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