低质量X射线双星的毫秒级准周期信号——最近的进展

最近对低质量X射线双星中的千赫兹准周期振动的研究表明 ,是辐射压力 ,而不是盘和磁球的相互作用以及处于盘内边界的广义相对论效应在短时标的盘切断机制上起作用。本文给出了一些研究结果及讨论。     

Fluxes of CO<Subscript>2</Subscript>, CH<Subscript>4</Subscript> and N<Subscript>2</Subscript>O from alpine grassland in the Tibetan Plateau

Using static chamber technique,fluxes of CO2,CH4 and N2O were measured in the alpine grassland area from July 2000 to July 2001,determinations of mean fluxes showed that CO2 and N2O were generally released from the soil,while the alpine grassland accounted for a weak CH4 sink.Fluxes of CO2,CH4 and N2O ranged widely.The highest CO2 emission occurred in August,whereas almost 90?of the whole year emission occurred in the growing season.But the variations of CH4 and N2O fluxes did not show any clear patterns over the one-year-experiment.During a daily variation,the maximum CO2 emission occurred at 16:00,and then decreased to the minimum emission in the early morning.Daily pattern analyses indicated that the variation in CO2 fluxes was positively related to air temperatures(R^2=0.73)and soil temperatures at a depth of 5 cm(R^2=0.86),whereas daily variations in CH4 and N2O fluxes were poorly explained by soil temperatures and climatic variables.CO2 emissions in this area were much lower than other grasslands in plain areas.     

The Non-Linear Stability of L4 in the Restricted Three-Body Problem when the Bigger Primary is a Triaxial Rigid Body

The non-linear stability of L ₄ in the restricted three-body problem has been studied when the bigger primary is a triaxial rigid body with its equatorial plane coincident with the plane of motion. It is found that L ₄ is stable in the range of linear stability except for three mass ratios:

1-（4-硝基苯基）-3-（3，5-二溴吡啶）三氮烯的合成及其与镍的显色反应

合成了1-(4-硝基苯基)-3-(3,5-二溴吡啶)三氮烯(NPDBPDT),并研究了NPD-BPDT与镍的显色反应。在pH 10.0的Na2B4O7-NaOH缓冲溶液介质中,表面活性剂Triton X-100存在下,镍与试剂生成摩尔比为1∶4的络合物在470 nm处有最大正吸收峰,表观摩尔吸光系数为1.02×105L.mol-1.cm-1;在540 nm处有最大负吸收峰,表观摩尔吸光系数为1.15×105L.mol-1.cm-1;以540 nm为参比波长、470 nm为测量波长进行双波长测定,表观摩尔吸光系数为2.17×105L.mol-1.cm-1。镍含量在0~480μg/L内符合比尔定律。方法用于合金样品中镍的测定,结果与原子吸收法相符,加标回收率为98.0%~102.0%;精密度小于5%(RSD,n=6)。     

华北平原冬麦田土壤CH4的吸收特征研究

利用静态箱/气相色谱(GC)法,对华北平原冬小麦拔节-成熟期间麦田土壤CH₄气体通量进行了测定,得出华北平原典型冬麦田土壤是大气CH₄的弱吸收汇。试验期间土壤CH₄通量存在明显的季节变化和日变化,麦田拔节-成熟期间土壤CH₄通量日平均值为-18.3μg·m^-2·h^-1,波动范围为-4.3-24.4μg·m^-2·h^-1;在土壤CH₄通量的日变化中,观测到麦田土壤在午间和夜间都有一个吸收峰,峰值出现的时间因生育期不同而有所不同。试验期间CH₄通量日平均值与土壤温度关系不明显,而与土壤水分呈负相关(α=0.01);日变化中土壤CH₄通量与地表温度的相关性较差,而与5cm地温相关密切。麦田拔节-成熟期间土壤CH₄通量日平均值随NH4+-N施用量的增加呈递减规律,农田秸秆还田后不利于土壤对CH₄的吸收。     

Carbon isotope ratios of C_4 plants in loess areas of North China

Recent stable carbon isotope studies have shown that the occurrence of C4 plants on the Earth was much later than that of C3 plants and there was a global ex-pansion of C4 biomass around 5―8 million years ago[1]. Although far fewer species use the C4 pat…     

甘肃省礼县马泉金矿床四号矿带地质特征及找矿潜力

马泉金矿床是受近EW向礼县-白云-山阳区域性深大断裂南支——礼县-洮坪断裂或层间挤压破碎带控制的中-低温热液矿床,目前已发现9个矿带。通过对其中四号矿带的勘查验证,对四号矿带的地质特征进行了重新认识和归纳总结。研究认为,矿带断裂构造十分发育,在矿区内发育的三条主要断裂构造严格控制着四号矿带的三条金矿体的空间展布及产出规模,找矿标志较多且明显,并认为,四号矿带之东西两侧延伸部位及其深部尚有一定的找矿潜力。     

C02-CH4流体与金成矿作用：以阿尔泰山南缘和穆龙套金矿为例

造山型金矿的成矿作用与H20-CO2流体有着密切的联系。然而对阿尔泰山南缘和穆龙套金矿的流体包裹体研究表明，无水的CO2-CH4流体在中亚成矿域中一些金矿床中具有同样重要意义。阿尔泰山南缘萨热阔布金矿包裹体的Xch4达0.20～0.23，穆龙套金矿的XCH4为0.07～0.23。CH4扩大了流体不混溶的范围，有利于对Au的富集沉淀。CO2流体在Au成矿中的重要作用至少包括了三方面的意义，即：缓冲流体PH值范围、提高流体中的Au含量并使其维持与还原硫的络合作用进行迁移；扩大超临界流体的温度范围；增加流体不混溶的区域。CH4的加入扩大了流体不混溶的范围，有利于对Au的富集沉淀。     

Calcium isotope fractionation in coccoliths of cultured Calcidiscus leptoporus, Helicosphaera carteri, Syracosphaera pulchra and Umbilicosphaera foliosa

Four species of marine calcifying algae, the coccolithophores Calcidiscus leptoporus, Helicosphaera carteri, Syracosphaera pulchra and Umbilicosphaera foliosa were grown in laboratory cultures under temperatures varying between 14 and 23 °C, and one species, C. leptoporus, under varying [CO₃²⁻], ranging from 105 to 219 μmol/kg. Calcium isotope compositions of the coccoliths resemble in both absolute fractionation and temperature sensitivity previous calibrations of marine calcifying species e.g. Emiliania huxleyi (coccolithophores) and Orbulina universa (planktonic foraminifera) as well as inorganically precipitated CaCO₃, but also reveal small species specific differences. In contrast to inorganically precipitated calcite, but similar to E. huxleyi and O. universa, the carbonate ion concentration of the medium has no statistically significant influence on the Ca isotope fractionation of C. leptoporus coccoliths; however, combined data of E. huxleyi and C. leptoporus indicate that the observed trends might be related to changes of the calcite saturation state of the medium. Since coccoliths constitute a significant portion of the global oceanic CaCO₃ export production, the Ca isotope fractionation in these biogenic structures is important for defining the isotopic composition of the Ca sink of the ocean, one of the key parameters for modelling changes to the marine Ca budget over time. For the present ocean our results are in general agreement with the previously postulated and applied mean value of the oceanic Ca sink (Δ_sed) of about − 1.3‰, but the observed inter- and intra-species differences point to possible changes in Δ_sed through earth history, due to changing physico-chemical conditions of the ocean and shifts in floral and faunal assemblages.