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961.
Chang Qing Luo Xiao Bin Zhang Li Cai Deng Yang Ping Luo Zhi Quan Luo Shu Zheng Yang 《Astrophysics and Space Science》2010,327(1):9-17
The long-term orbital period changes of a large sample of detached chromospherically active binaries (CABs) were studied. Eleven such systems were found to be undergoing secular period decreases with the rates of ?6.3×10?9 to ?1.1×10?6 days per year. The period decreasing rates are found to vary depending on the orbital period. The longer the orbital period is, the more rapidly the period decreases. Following Stepien (Mon. Not. R. Astron. Soc. 274:1019, 1995), the period decreasing rate predicted by angular momentum loss (AML) caused by magnetic wind is computed for each system. A comparison between the observed and calculated period decreasing rates shows that the former values are obviously larger than the latter by 1–3 orders of magnitude. It suggests that the magnetic wind is not likely the determinant mechanism driving the AML in these systems. Finally, the orbital angular momentum (AM) and the rate of AML, $\dot{J}$ , are computed for each system. It shows that the AM have a similar change with the orbital period like dP/dt does, but $\log\dot{J}/J$ presents no strict changing with the kinematical ages. 相似文献
962.
Rainfall effects on wind waves and turbulence are investigated through the laboratory experiments in a large wind-wave tank. It is found that the wind waves are damped as a whole at low wind speeds, but are enhanced at high wind speeds. This dual effect of rain on the wind waves increases with the increase of rain rate, while the influence of rainfall-area length is not observable. At the low wind speed, the corresponding turbulence in terms of the turbulent kinetic energy (TKE) dissipation rate is significantly enhanced by rain- fall as the waves are damped severely. At the high wind speed, the augment of the TKE dissipation rate is suppressed while the wind waves are enhanced simultaneously. In the field, however, rainfall usually hin- ders the development of waves. In order to explain this contradiction of rainfall effect on waves, a possibility about energy transfer from turbulence to waves in case of the spectral peak of waves overlapping the inertial subrange of turbulence is assumed. It can be applied to interpret the damping phenomenon of gas trans- fer velocity in the laboratory experiments, and the variation of the TKE dissipation rates near sea surface compared with the law of wall. 相似文献
963.
通过"双三次曲面拟合—时间步长积分—双三次曲面拟合……",实现成为一种双三次曲面拟合新算法数值模式。它对模式大气作非线性(空间二阶可导)描述,是用数值分析(三次样条/双三次曲面)与计算方法近似求解大气运动非线性偏微分方程组。用Z坐标系高分辨率双三次数值模式,采用原始大气运动方程组和采用欧拉时间积分方案,设置理想扰动,对大气声波Lamb波做数值模拟;采用大气不可压假定,除去声波,对大气重力波龙卷扰动做数值模拟。对比模拟发现:理想Lamb波以声速在水平方向传播,扰动能量频散快,仅能在原地持续数秒钟;理想龙卷扰动则在原地可持续约1 min,且波动内圈(外圈)自下至上始终处于风场辐合(辐散)状态,具冷心结构和气压驻波特征,可因水汽进入扰动与借助凝结潜热释放而得到发展。 相似文献
964.
Orhan Karsli Abdurrahman Dokuz İbrahim Uysal Faruk Aydin Bin Chen Raif Kandemir Jan Wijbrans 《Contributions to Mineralogy and Petrology》2010,160(4):467-487
We present elemental and Sr–Nd–Pb isotopic data for the magmatic suite (~79 Ma) of the Harşit pluton, from the Eastern Pontides
(NE Turkey), with the aim of determining its magma source and geodynamic evolution. The pluton comprises granite, granodiorite,
tonalite and minor diorite (SiO2 = 59.43–76.95 wt%), with only minor gabbroic diorite mafic microgranular enclaves in composition (SiO2 = 54.95–56.32 wt%), and exhibits low Mg# (<46). All samples show a high-K calc-alkaline differentiation trend and I-type
features. The chondrite-normalized REE patterns are fractionated [(La/Yb)
n
= 2.40–12.44] and display weak Eu anomalies (Eu/Eu* = 0.30–0.76). The rocks are characterized by enrichment of LILE and depletion
of HFSE. The Harşit host rocks have weak concave-upward REE patterns, suggesting that amphibole and garnet played a significant
role in their generation during magma segregation. The host rocks and their enclaves are isotopically indistinguishable. Sr–Nd
isotopic data for all of the samples display I
Sr = 0.70676–0.70708, ε
Nd(79 Ma) = −4.4 to −3.3, with T
DM = 1.09–1.36 Ga. The lead isotopic ratios are (206Pb/204Pb) = 18.79–18.87, (207Pb/204Pb) = 15.59–15.61 and (208Pb/204Pb) = 38.71–38.83. These geochemical data rule out pure crustal-derived magma genesis in a post-collision extensional stage
and suggest mixed-origin magma generation in a subduction setting. The melting that generated these high-K granitoidic rocks
may have resulted from the upper Cretaceous subduction of the Izmir–Ankara–Erzincan oceanic slab beneath the Eurasian block
in the region. The back-arc extensional events would have caused melting of the enriched subcontinental lithospheric mantle
and formed mafic magma. The underplating of the lower crust by mafic magmas would have played a significant role in the generation
of high-K magma. Thus, a thermal anomaly induced by underplated basic magma into a hot crust would have caused partial melting
in the lower part of the crust. In this scenario, the lithospheric mantle-derived basaltic melt first mixed with granitic
magma of crustal origin at depth. Then, the melts, which subsequently underwent a fractional crystallization and crustal assimilation
processes, could ascend to shallower crustal levels to generate a variety of rock types ranging from diorite to granite. Sr–Nd
isotope modeling shows that the generation of these magmas involved ~65–75% of the lower crustal-derived melt and ~25–35%
of subcontinental lithospheric mantle. Further, geochemical data and the Ar–Ar plateau age on hornblende, combined with regional
studies, imply that the Harşit pluton formed in a subduction setting and that the back-arc extensional period started by least
~79 Ma in the Eastern Pontides. 相似文献
965.
大别山岳西县石关混合岩锆石SHRIMP定年及其地质意义 总被引:1,自引:1,他引:0
安徽岳西县石关混合岩属于原北大别变质杂岩的一部分。锆石SHRIMPU-Pb定年结果:第一次变质时间为232Ma,相当于晚三叠世早期,第二次变质时间为207Ma,相当于晚三叠世晚期。复合锆石的核部(继承锆石)为发育韵律环带的岩浆碎屑锆石,其年龄值分别为560Ma、444Ma、394Ma、378Ma和331Ma,暗示其原岩非岩浆岩,而应为沉积岩;研究结果还表明,北大别石关混合岩经历了两次变质作用:①超高压变质作用,变质时间为232Ma(n=5加权平均年龄);②退变质作用,时间为207Ma。与苏鲁地区超高压变质和退变质时间一致。 相似文献
966.
广西新元古代BIF的铁同位素特征及其地质意义 总被引:10,自引:1,他引:9
通过分析广西三江地区新元古代条带状含铁建造的Fe同位素和主量元素组成,对海水的氧化还原状态提供了制约,为富禄期的地球处于间冰期提供了证据。相对于标准物质IRMM-014,新元古代含铁建造不同条带全岩样品的δ57Fe值变化范围1.60‰~2.20‰,平均值为1.85‰,表明BIF样品富集铁的重同位素。条带状含铁建造主要由Fe2O3和SiO2组成,但却具有较高的Al2O3含量。这表明条带状含铁建造样品不是纯净的化学沉积物,而是具有一定的碎屑物质输入。碎屑输入量的不同引起深色和浅色条带之间铁同位素组成存在着0.4‰的差别。剔除碎屑的影响,新元古代BIF从海水中沉淀的赤铁矿δ57Fe的平均值在2‰左右,略高于太古代条带状铁建造的Fe同位素组成,这表明当时海水的氧逸度可能比太古代还低。这说明在富禄期绝大部分海洋仍旧被冰盖覆盖,只在局部出现融化。因此,富禄期的地球可能出于冰期的相对温暖阶段,而不是间冰期。 相似文献
967.
安徽庐枞火山岩盆地橄榄玄粗岩系的地球化学特征及其对下扬子地区晚中生代岩石圈减薄机制的约束 总被引:17,自引:2,他引:15
庐枞盆地内的中生代火山-潜火山岩具高钾和相对富碱为特性,属典型的橄榄玄粗岩系列。它们在地球化学上表现出明显富集Rb、Th、U、K等强不相容元素和轻稀土元素,亏损高场强元素Nb和Ta的特征。Nd、Sr同位素组成总体位于富集型的扬子克拉通岩石圈地幔的范围内或其附近,显示其母岩浆主要是由富集型地幔部分熔融形成的。火山-潜火山岩的成分变异趋势显示橄榄玄粗质幔源岩浆在高压下(斜长石稳定压力之下,1.5GPa)经历过以单斜辉石和钛铁氧化物为主的矿物分离结晶作用。低压下矿物的分离结晶作用及上地壳物质的混染则不明显。这套火山-潜火山岩的部分地球化学性质(如Ce/Yb比值)类似于大洋岛弧内的橄榄玄粗岩,可能意味着区内由于岩石圈的减薄,软流圈地幔上涌到了岩石圈相对较浅的部位,控制源区部分熔融的主要是尖晶石相地幔岩。虽然局部(如靠近郯庐断裂的盆地西缘)可能存在着明显的热侵蚀,但"突发性的"机械拆沉是区内(乃至整个长江中下游地区)岩石圈减薄的主要机制。在整个晚中生代岩石圈减薄的过程中,这两种机制可能一直相互促进着。 相似文献
968.
969.
讨论了磁源TEM中心回线装置全程视电阻率的计算问题。利用电偶极子的瞬变场叠加来计算磁源TEM中心回线装置的瞬变场,均匀半空间的计算结果表明,该方法是可行的。用电偶极子的瞬变场定义了磁源瞬变电磁法中心回线装置全程视电阻率,通过对二、三、四层电性断面的视电阻率的计算,并与TEM晚期视电阻率进行了对比,说明了该定义的优越性。实测磁源TEM资料的计算表明,用电偶极子的瞬变场定义的磁源瞬变电磁法中心回线装置全程视电阻率较好地反映了电性断面特征,其对浅层磁源TEM探测及资料解译具有使用价值。 相似文献
970.