Clouds, hazes, and the stratospheric methane abundance in Neptune

Analysis of high-spatial-resolution (approximately 0.8 arcsec) methane band and continuum imagery of Neptune's relatively homogeneous Equatorial Region yields significant constraints on (1) the stratospheric gaseous methane mixing ratio (fCH4,s), (2) the column abundances and optical properties of stratospheric and tropospheric hydrocarbon hazes, and (3) the wavelength-dependent single-scattering albedo of the 3-bar opaque cloud. From the center-to-limb behavior of the 7270-angstroms and 8900-angstrom sCH4 bands, the stratospheric methane mixing ratio is limited to fCH4,s < 1.7 x 10(-3), with a nominal value of fCH4,s = 3.5 x 10(-4), one to two orders of magnitude less than pre-Voyager estimates, but in agreement with a number of recent ultraviolet and thermal infrared measurements, and largely in agreement with the tropopause mixing ratio implied by Voyager temperature measurements. Upper limits to the stratospheric haze mass column abundance and 6190-angstroms and 8900-angstroms haze opacities are 0.61 microgram cm-2 and 0.075 and 0.042, respectively, with nominal values of 0.20 microgram cm-2 and 0.025 and 0.014 for the 0.2-micrometer radius particles preferred by the recent Voyager PPS analysis of Pryor et al. (1992, Icarus 99, 302-316). The tropospheric CH4 haze opacities are comparable to that found in the stratosphere, upper limits of 0.104 and 0.065 at 6190 angstroms and 8900 angstroms, respectively, with nominal values of 0.085 and 0.058. This indicates a column abundance less than 11.0 micrograms cm-2, corresponding to the methane gas content within a well-mixed 3% methane tropospheric layer only 0.1 cm thick near the 1.5-bar CH4 condensation level. Constraints on the single-scattering albedos of these hazes include (1) for the stratospheric component, 6190-angstroms and 8900-angstroms imaginary indices of refraction less than 0.047 and 0.099, respectively, with 0.000 (conservative scattering) being the nominal value at both wavelengths, and (2) CH4 haze single-scattering albedos greater than 0.85 and 0.50 at these two wavelengths, with conservative scattering again begin the preferred value. However, conservative scattering is ruled out for the opaque cloud near 3 bars marking the bottom of the visible atmosphere. Specifically, we find cloud single-scattering albedos of 0.915 +/- 0.006 at 6340 angstroms, 0.775 +/- 0.012 at 7490 angstroms, and 0.803 +/- 0.010 at 8260 angstrom. Global models utilizing a complete global spectrum confirm the red-absorbing character of the 3-bar cloud. The global-mean model has approximately 7.7 times greater stratospheric aerosol content then the Equatorial Region. An analysis of stratospheric haze precipitation rates indicates a steady-state haze production rate of 0.185-1.5 x 10(-14) g cm-2 sec-1, in agreement with recent theoretical photochemical estimates. Finally, reanalysis of the Voyager PPS 7500-angstroms phase angle data utilizing the fCH4,s value derived here confirms the Pryor et al. result of a tropospheric CH4 haze opacity of a few tenths in the 22-30 degrees S latitude region, several times that of the Equatorial Region or of the globe. The factor-of-10 reduction in fCH4,s below that assumed by Pryor et al. implies decreased gas absorption and consequently a decrease in the forward-scattering component of tropospheric aerosols.     

Fractionation of carbon isotopes by phytoplankton and estimates of ancient CO2 levels

Reports of the 13C content of marine particulate organic carbon are compiled and on the basis of GEOSECS data and temperatures, concentrations, and isotopic compositions of dissolved CO2 in the waters in which the related phytoplankton grew are estimated. In this way, the fractionation of carbon isotopes during photosynthetic fixation of CO2 is found to be significantly correlated with concentrations of dissolved CO2. Because ancient carbon isotopic fractionations have been determined from analyses of sedimentary porphyrins [Popp et al., 1989], the relationship between isotopic fractionation and concentrations of dissolved CO2 developed here can be employed to estimate concentrations of CO2 dissolved in ancient oceans and, in turn, partial pressures of CO2 in ancient atmospheres. The calculations take into account the temperature dependence of chemical and isotopic equilibria in the dissolved-inorganic-carbon system and of air-sea equilibria. Paleoenvironmental temperatures for each sample are estimated from reconstructions of paleogeography, latitudinal temperature gradients, and secular changes in low-latitude sea surface temperature. It is estimated that atmospheric partial pressures of CO2 were over 1000 micro atm 160 - 100 Ma ago, then declined to values near 300 micro atm during the next 100 Ma. Analysis of a high-resolution record of carbon isotopic fractionation at the Cenomanian-Turonian boundary suggests that the partial pressure of CO2 in the atmosphere was drawn down from values near 840 micro atm to values near 700 micro atm during the anoxic event.     

地球化学异常再现性与可对比性

不同密度采样是否可以获得稳定的和可追索的地球化学模式是检验采样是否具有代表性，分析技术是否成熟的重要依据。笔者选择新疆哈密大南湖地区约6400km^2面积，进行了从超低密度(1个样／100km^2)，甚低密度(1个样／25km^2)直到低密度(1个样／4km^2)地球化学采样，对比了3种密度地球化学采样所获得的地球化学数据和异常分布模式。得出如下结论：超低密度、甚低密度、低密度地球化学调查获得的元素含量平均值和背景值非常接近；超低密度、甚低密度、低密度调查所圈定的地球化学省在形态上和变化趋势上非常相似，浓集中心的位置重合，表明不同调查阶段可获得稳定的和可追索的地球化学模式；采样密度越大数据离散程度越高，即最小值更小，最大值更大，表明元素分布的局部不均匀性，正是这种局部的不均匀性才能通过加密采样刻画出地球化学模式的细节变化，为逐步追踪矿化体奠定了基础；超低密度和甚低密度采样可以有效圈定矿集区所形成的大规模地球化学异常，低密度地球化学调查不仅可以圈定矿集区异常，同时可以圈定分散矿化的小规模局部异常。     

应用岩石化学元素丰度研究地球化学块体

应用岩石化学元素丰度研究地球化学块体,探讨地球化学块体中元素组成的差异.对中国东部岩石地球化学块体研究表明,华南分布着的巨大的W, Sn, Mo, Bi, U, Th, Pb, Li, Rb, Cs, Be, Nb, Ta, HREE, Y及Tl, Cd, F, K岩石地球化学域,其中的岩石地球化学块体是形成水系沉积物地球化学块体和大型矿集区的主要物质来源.该研究不仅丰富了地球化学块体理论,而且以新的视野从宏观角度上为勘查地球化学、理论地球化学、成矿学与找矿学、环境地学、大地构造学提供有价值的基础性研究资料.     

中国火成岩化学元素的丰度与分布

在中国各构造单元构选采了１０３６４件火成岩样品合成１１３１个分析样，采用仪器中子活化法，Ｘ射线荧光光谱法，原子吸收法，原子荧光光谱法，催化波极谱法和分光光度法等１５种可靠分析方法进行测试，对一些难测痕量元素采用了最新的分析研究成果，以同类国家一级标准物质监控分析质量。     

中国东部上地壳化学组成

在中国东部(东经105°以东)约计330万km~2系统采集了28253个岩石样品,组合成2718件分析样,选用了15种可靠的分析方法,以国家一级标准物质监控分析质量,提出了76种化学元素在中国东部出露地壳、沉积盖层、出露基底和上地壳的平均化学组成.     

中国东部大陆岩石地球化学图揭示的信息

根据中国东部各省(区、市)区域地质志、1∶50万地质图和中国东部地壳与岩石元素丰度研究成果首次编制的中国东部60种元素的岩石地球化学图,基本反映了与特定岩性有关的区域岩石地球化学元素含量分布特征和与大地构造单元有关的区域地球化学元素含量分布特征,直观表达了中国东部空间地理上元素背景含量的宏观分布与变化,以及不同大地构造单元元素背景含量的变化趋势。这一成果为勘查地球化学、环境地球化学,特别是区域化探扫面水系沉积物资料的定量解释提供了基本依据,为基础地质、大地构造、区域成矿研究提供了重要资料,也为地球化学块体理论及其形成机制的研究提供了强有力的支持。     

中国东部大陆岩石地球化学图揭示的信息

根据中国东部各省(区、市)区域地质志、1:50万地质图和中国东部地壳与岩石元素丰度研究成果首次编制的中国东部60种元素的岩石地球化学图,基本反映了与特定岩性有关的区域岩石地球化学元素含量分布特征和与大地构造单元有关的区域地球化学元素含量分布特征,直观表达了中国东部空间地理上元素背景含量的宏观分布与变化,以及不同大地构造单元元素背景含量的变化趋势.这一成果为勘查地球化学、环境地球化学,特别是区域化探扫面水系沉积物资料的定量解释提供了基本依据,为基础地质、大地构造、区域成矿研究提供了重要资料,也为地球化学块体理论及其形成机制的研究提供了强有力的支持.     

兴蒙造山带—华北克拉通地球化学走廊带沉积物主成分的含量与空间分布研究

选取兴蒙造山带—华北克拉通地球化学走廊带上沉积物的SiO_2、Al_2O_3、CaO、MgO、Na_2O、K_2O、TFe_2O_3、FeO、TiO_2、MnO、P_2O_5、CO_2、H_2O~+、pH十四个指标,研究其在不同二级构造单元、地理景观、土壤类型、降雨量等级下的含量与空间分布特征,并讨论该地球化学走廊带上化学蚀变指数。结果表明:在兴蒙造山带—华北克拉通地球化学走廊带上,作为沉积物主体的SiO_2、Al_2O_3两者含量为明显负相关而空间分布表现出此消彼长的特征;CaO、MgO、CO_2高含量分布区则与碳酸盐岩地层或含碳酸盐矿物的土壤有关,而MgO的高含量还与走廊带上镁铁质基性-超基性岩有一定关系,表明了这三个指标的高含量受特定岩性或矿物的影响较大;Na_2O、K_2O含量除了受继承的基岩影响外,还受到后期的风化作用和气候及自身地球化学性质等复杂因素综合影响,对Na_2O来说尤为如此;TFe_2O_3、MnO、TiO_2、P_2O_5相对于在地质背景复杂地段,经过冲积平原的沉积物混匀后,含量差异更小;相对干冷的内蒙古半干旱草原的气候条件有利于FeO存在,使得其相对燕山地区含量差异较TFe_2O_3要小,在章丘以南相对温暖湿润地区更易被氧化而导致其含量整体较低;北方干冷气候条件下,沉积物H_2O~+含量普遍较低,局部高含量位于碳酸盐岩地层或第四系分布区;走廊带上的pH值反映了沉积物偏碱性的特征,而在章丘以南的地区随着降雨量的增加,相对温暖湿润的气候条件,沉积物pH值表现为中性-偏弱酸性;兴蒙造山带—华北克拉通地球化学走廊带沉积物的CIA值反映出在寒冷、干燥气候条件下低等的化学风化程度,兴蒙造山带沉积物平均风化程度相对华北克拉通沉积物的平均风化程度差异变化相对要小,显示兴蒙造山带的降雨量与温度等风化影响因素变化较小。作为反映元素的地球化学亲和性的量化指标,离子电位可以更好地帮助理解沉积物元素的含量和空间分布差异。     

地球化学块体与大型矿集区的关系——以东天山为例

通过在东天山15万km2的战略性深穿透地球化学调查共圈出大于1000km2以上的地球化学块体18处,其中铜-铅-锌-银地球化学块体5处,铜地球化学块体3处,铜-镍地球化学块体1处,金的地球化学块体4处,铀的地球化学块体3处,铂-钯地球化学块体1处,钨地球化学块体1处。有6处地球化学块体与已知矿集区相对应,新圈定的地球化学块体12处,其中有3处发现了新的矿床。根据这些块体与矿集区的对比得出如下结论:所有的已知矿集区都位于地球化学块体的范围之内,地球化学块体为矿集区的形成提供了丰富的物质基础;有矿集区的存在一定有地球化学块体的存在,但反过来有地球化学块体的存在不一定有矿集区的存在,地球化学块体是客观存在的,而矿集区是已经发现了一系列矿床并勘探到一定程度才能称作矿集区,因此,地球化学块体内可能会存在潜在的矿集区,这为利用地球化学块体预测新的矿集区提供了依据。