An XMM–Newton observation of the neutron star X-ray transient 2S 1803−245 in quiescence

We observed the neutron star X-ray transient 2S 1803−245 in quiescence with the X-ray satellite XMM–Newton , but did not detect it. An analysis of the X-ray bursts observed during the 1998 outburst of 2S 1803−245 gives an upper limit to the distance of ≤7.3 kpc, leading to an upper limit on the quiescent 0.5–10 keV X-ray luminosity of  ≤2.8 × 10³² erg s⁻¹  (3σ). Since the expected orbital period of 2S 1803−245 is several hours, this limit is not much higher than those observed for the quiescent black hole transients with similar orbital periods.     

海拉尔盆地乌尔逊凹陷幔源CO2充注对下白垩统砂岩储层质量的影响

海拉尔盆地乌尔逊凹陷下白垩统含片钠铝石砂岩部分记录了幔源CO_2-砂岩相互作用历史.为揭示幔源CO_2充注对储层质量的影响,通过偏光显微镜、扫描电镜观察和孔隙度、渗透率数据研究了海拉尔盆地乌尔逊凹陷含片钠铝石砂岩的岩石学和储层特征.幔源CO_2的充注导致了长石的部分溶解和片钠铝石及铁白云石的沉淀.长石的溶解形成了次生孔隙.片钠铝石以针状晶形为特征,其集合体呈束状、簇状、扇状和玫瑰花状.部分片钠铝石呈板状.片钠铝石以充填孔隙为主,少量交代长石和其他骨架碎屑颗粒.片钠铝石局部被铁白云石交代,说明铁白云石的形成晚于片钠铝石.片钠铝石的含量为1%～20%.相同深度段的含片钠铝石砂岩(n=597,h=1309.15～2140.71m)与普通砂岩(n=1550,h=1323.72～2141.3m)的孔隙度、渗透率数据统计表明,含片钠铝石砂岩的物性整体上低于普通砂岩,说明CO_2的充注导致了储层质量的改变.片钠铝石含量-孔隙度和片钠铝石含量-渗透率之间的关系,揭示片钠铝石含量是引起储层质量改变的主要因素.片钠铝石含量10%似乎是储层质量发生变化的界限,当片钠铝石含量＞10%,随片钠铝石含量增加,砂岩的孔隙度和渗透率降低;当片钠铝石含量＜10%,随片钠铝石含量增加,部分砂岩的孔隙度和渗透率表现出增加趋势.作者认为,片钠铝石含量高的砂岩长期处于高CO_2分压成岩环境,而片钠铝石含量低的砂岩则处于高CO_2分压成岩环境的时间相对较短.     

雷琼地区晚新生代玄武岩地球化学：EM2成分来源及大陆岩石圈地幔的贡献

对雷琼地区21个晚新生代玄武岩样品的主量、微量元素和Sr、Nd、Pb同位素分别用湿化学法、ICP-MS和MC-ICPMS进行了测定.这些玄武岩主要为石英拉斑玄武岩,其次为橄榄拉斑玄武岩和碱性玄武岩.大多数样品的微量元素和同位素成分与洋岛玄武岩(OIBs)相似,而且随着SiO_2不饱和度增加,不相容元素含量也增加.除R4-1可能受到地壳混染外,其他样品相对均一的Nd同位素(ε_(Nd)=2.5-6.0)以及变化明显但范围有限的Sr同位素(0.703106～0.704481),可能继承了地幔源区的特征.~(87)Sr/~(86)Sr与~(206)Pb/~(204)Pb的正相关和~(143)Nd/~(144)Nd与~(206)Pb/~(204)Pb的负相关特征暗示DM(软流圈地幔)与EM2(岩石圈地幔)的混合.地幔捕虏体的同位素特征暗示EM2成分不可能存在于尖晶石橄榄岩地幔,而La/Yb和Sm/Yb系统表明岩浆由石榴石橄榄岩部分熔融产生,这意味着EM2成分可能存在于石榴石橄榄岩地幔.雷琼地区玄武岩的地球化学变化可以用软流圈地幔为主的熔体加入不同比例石榴石橄榄岩地幔不同程度熔融产生的熔体来解释:碱性玄武岩和橄榄拉斑玄武岩是软流圈熔体与石榴石橄榄岩地幔较低程度(7%～9%)熔融体混合,而石英拉斑玄武岩是软流圈熔体与石榴石橄榄岩地幔较高程度(10%～20%)熔融体的混合.     

Oxidation of CO on surface hematite in high CO2 atmospheres

We propose a mechanism for the oxidation of gaseous CO into CO₂ occurring on the surface mineral hematite (Fe₂O₃(s)) in hot, CO₂-rich planetary atmospheres, such as Venus. This mechanism is likely to constitute an important source of tropospheric CO₂ on Venus and could at least partly address the CO₂ stability problem in Venus’ stratosphere, since our results suggest that atmospheric CO₂ is produced from CO oxidation via surface hematite at a rate of 0.4 petagrammes (Pg) CO₂ per (Earth) year on Venus which is about 45% of the mass loss of CO₂ via photolysis in the Venusian stratosphere. We also investigated CO oxidation via the hematite mechanism for a range of planetary scenarios and found that modern Earth and Mars are probably too cold for the mechanism to be important because the rate-limiting step, involving CO(g) reacting onto the hematite surface, proceeds much slower at lower temperatures. The mechanism may feature on extrasolar planets such as Gliese 581c or CoRoT-7b assuming they can maintain solid surface hematite which, e.g. starts to melt above about 1200 K. The mechanism may also be important for hot Hadean-type environments and for the emerging class of hot Super-Earths with planetary surface temperatures between about 600 and 900 K.     

Estimates of global M_2 internal tide energy fluxes using TOPEX/POSEIDON altimeter data

TOPEX/POSEIDON altimeter data from October 1992 to June 2002 are used to calculate the global barotropic M2 tidal currents using long-term tidal harmonic analysis. The tides calculated agree well with ADCP data obtained from the South China Sea (SCS). The maximum tide velocities along the semi-major axis and semi-minor axis can be computed from the tidal ellipse. The global distribution of M2 internal tide vertical energy flux from the sea bottom is calculated based on a linear internal wave generation model. The global vertical energy flux of M2 internal tide is 0.96 TW, with 0.36 TW in the Pacific, 0.31 TW in the Atlantic and 0.29 TW in the Indian Ocean, obtained in this study. The total horizontal energy flux of M2 internal tide radiating into the open ocean from the lateral boundaries is 0.13 TW, with 0.06 TW in the Pacific, 0.04TW in the Atlantic, and 0.03 TW in the Indian Ocean. The result shows that the principal lunar semi-diurnal tide M2 provides enough energy to maintain the large-scale thermohaline circulation of the ocean.     

珠江河口经济动物体铜铅锌镉的含量

分别于2000年4月、2001年4月和2002年8月对珠江河口水域海洋经济动物体内Cu、Pb、Zn、Cd四种重金属元素的含量进行了调查分析,结果表明,14种经济动物体肌肉Cd、Cu、Pb、Zn各元素的平均含量分别是0.08、2.67、0.05、5.69mg·kg~(-1),其变化范围为nd～0.46mg·kg~(-1)、0.24～11.85mg·kg~(-1)、nd～0.26mg·kg~(-1)、1.55～18.36mg·kg~(-1)。甲壳类与头足类生物体内铜铅锌镉含量比较接近,远远高于鱼类的含量。所检测的14种经济类海洋动物中,虾姑、乌贼Cu的含量高于其余三种元素的含量,其余12种生物Zn的含量比另三种元素含量高。三次调查该水域经济类海洋动物体铜铅锌镉的含量基本一致。与水产品中有毒有害物质限量标准比较,14种被测样品铜、铅和镉的含量全部符合该标准的要求。     

CryoSat-2卫星海冰区域波形识别及海冰干舷高确定

利用40%阈值法对CryoSat-2卫星波形数据进行重跟踪,将波形特征参数和海冰浓度相结合,对海冰和Lead(浮冰之间的开阔水域)进行有效识别。利用沿轨前后搜索算法计算海冰干舷高,并引用AWI结果,绘制2011~2013年北冰洋多年冰区域和一年冰区域平均海冰干舷高变化趋势图。比较本文结果与AWI结果的各年同期数据,验证本文结果的可靠性。     

山东省兰陵县车辋地区铜铅多金属矿地质特征及找矿标志

车辋地区铜铅多金属矿区位于山东省兰陵县车辋镇东部,区内寒武奥陶纪碳酸盐岩地层分布广泛,中生代岩浆活动频繁,构造活动强烈、层间破碎带发育。激电异常明显,且具低阻高极化特征。铜铅多金属矿化期为岩浆期后热液阶段,岩体边部和外侧的构造破碎带、层间破碎带为成矿热液的运移、储存提供了有利空间,是寻找多金属矿的有利部位。     

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酸性流体对碳酸盐岩储层的改造作用

普遍认为CO2、有机酸及H2S是碳酸盐岩储层溶蚀作用的酸性流体。CO2对碳酸盐岩储层的溶蚀作用已有不少学者进行了研究,本文则以一个全新的模拟实验方式对不同类型碳酸盐岩在有机酸和H2S水溶液中的相对溶蚀能力进行了研究,结果发现随温度从常温升高至200℃,有机酸对碳酸盐岩的溶蚀能力由弱变强再变弱,在90℃左右溶蚀能力最强。而H2S水溶液对碳酸盐岩的溶蚀作用则明显不同,60℃时基本达到最大溶蚀率,温度继续升高后,溶蚀能力一直维持在较高的水平并略有增加,150℃后突然降低。由于H2S主要是硫酸盐高温热还原产物（TSR）,因而在碳酸盐岩成岩早期阶段,溶蚀作用的流体可能主要是有机酸和C02,而在深埋阶段,H2S水溶液则可能是溶蚀作用的主要流体。