Deep-sea hydrocarbon seep gastropod Bathynerita naticoidea responds to cues from the habitat-providing mussel Bathymodiolus childressi

Bathynerita naticoidea (Gastropoda: Neritidae) is a numerically dominant heterotrophic gastropod found at hydrocarbon seep sites on the upper Louisiana slope of the Gulf of Mexico. Snails of this species are commonly associated with beds of the methanotrophic mussel Bathymodiolus childressi (Bivalvia: Mytilidae), and their population structure mirrors that of the mussels they are found among. Previous studies have shown that these snails feed on bacteria and decomposing periostracum on the B. childressi shell. We predicted that B. naticoidea might be attracted to cues specific to its preferred habitat, such as dissolved methane, mucus from conspecific snails, or metabolites produced by B. childressi mussels. To examine this, we used a flow‐through Y‐maze system to investigate the behavior of B. naticoidea exposed to these potential cues. We found that the nerite is not attracted to methane, but is strongly attracted to seawater conditioned with B. childressi. The attractant appears to be specific to this type of mussel, and is not a soluble cue produced by conspecific snails.     

海洋沉积物中石英单矿物的化学分离

海洋沉积物中的石英作为陆源物质的标志性矿物,是古环境和古气候演化的信息载体,已成为古环境和古气候演化研究的重要替代指标.提供了改进了的化学分离海洋沉积物中石英单矿物的方法流程.在流程中的不同阶段可有效去掉全样中的生物组分、粘土矿物和长石等,取得海洋沉积物全样的总陆源矿物、石英+长石、石英的相对和绝对含量,通过计算可获得各种组分的通量,通过粒度分析可获得粒度数据.同一样品的17次重复实验表明,含量结果的平均相对误差仅为2.36%;显微镜和X射线衍射分析检查所分离出的石英纯度可达98%以上;激光粒度分析表明,化学试剂对石英的溶蚀作用不明显,不影响粒度分析结果.     

关中盆地潜水化学特征及其变化趋势

本文在阐明关中盆地环境水文地质条件的基础上,论述了关中盆地潜水化学特征及其成因,并着重对盆地潜水化学变化的几个主要问题,诸如常规组份的升高及水化学类型的改变、潜水硬度的升高、硝酸盐的富集及微量重金属元素的污染等进行了分析。讨论了上述问题的因果及今后工作意见。     

Darcys Law Expressed by Chemical Index

Ｉｎ 18 5 6 ,ＨｅｎｒｙＤａｒｃｙｐｕｂｌｉｓｈｅｄｈｉｓｌａｗ ,ｔｈｅＤａｒｃｙ’ｓｌａｗ ,ｅｘｐｒｅｓｓｅｄｂｙｈｙｄｒａｕｌｉｃｉｎｄｅｘｔｈｒｏｕｇｈａｌｏｎｇ ｔｅｒｍｅｘｐｅｒｉｍｅｎｔｏｆｗａｔｅｒｐｅｒｍｅａｔｉｏｎｉｎｍｕｌｔｉ ｍｉｎｅｒａｌｍｅｄｉｕｍ (Ｘｕ ,1986 ) ,ｗｈｉｃｈｎｏｔｏｎｌｙｍｅｔｔｈｅｕｒｇｅｎｔｎｅｅｄｏｆｔｈｅｄｅｖｅｌｏｐｍｅｎｔｏｆｓｏｃｉａｌｅｃｏｎｏ ｍｙａｎｄｐｒａｃｔｉｃｅｆｏｒｃａｌｃｕｌａｔｉｏｎｏｆｗｅｌｌｗａｔｅｒｑｕａｎｔｉｔｙａｔｔ…     

银河系化学演化研究进展

银河系的形成与演化是天体物理学研究的重大前沿课题,银河系的化学演化在其中更具有极其重要的地位。随着观测资料的不断积累和理论工作的不断深入,银河系化学演化的研究取得了一系列进展。在观测方面,从太阳附近区域,整个银盘,银晕和核球等方面简要回顾了银河系化学演化模型主要观测约束的近期结果;在化学演化模型方面,回顾了银河系化学演化研究的发展历程和近期进展,并对未来的研究进行了展望。     

Concentration–discharge relationships reflect chemostatic characteristics of US catchments

Concentration–discharge relationships have been widely used as clues to the hydrochemical processes that control runoff chemistry. Here we examine concentration–discharge relationships for solutes produced primarily by mineral weathering in 59 geochemically diverse US catchments. We show that these catchments exhibit nearly chemostatic behaviour; their stream concentrations of weathering products such as Ca, Mg, Na, and Si typically vary by factors of only 3 to 20 while discharge varies by several orders of magnitude. Similar patterns are observed at the inter‐annual time scale. This behaviour implies that solute concentrations in stream water are not determined by simple dilution of a fixed solute flux by a variable flux of water, and that rates of solute production and/or mobilization must be nearly proportional to water fluxes, both on storm and inter‐annual timescales. We compared these catchments' concentration–discharge relationships to the predictions of several simple hydrological and geochemical models. Most of these models can be forced to approximately fit the observed concentration–discharge relationships, but often only by assuming unrealistic or internally inconsistent parameter values. We propose a new model that also fits the data and may be more robust. We suggest possible tests of the new model for future studies. The relative stability of concentration under widely varying discharge may help make aquatic environments habitable. It also implies that fluxes of weathering solutes in streams, and thus fluxes of alkalinity to the oceans, are determined primarily by water fluxes. Thus, hydrology may be a major driver of the ocean‐alkalinity feedback regulating climate change. Copyright © 2009 John Wiley & Sons, Ltd.     

Macroalgae in a spring stream in Shanxi Province： composition and relation to physical and chemical variables

Fourteen stream segments were investigated throughout the Xin’an Spring in Shanxi Province, China in 2004. The variation ranges in stream size, current velocity, discharge, dissolved oxygen, and specific conductance were large. Twenty-two macroalgae species were found in the stream. Major divisions in terms of species numbers were Chlorophyta (59.1%), Cyanophyta (22.8%), Xanthophyta (9.1%), Rhodophyta (4.5%) and Charophyta (4.5%). The most widespread species, Cladophora rivularis (50.0%), also Oedogonium sp. (42.9%) and Spirogyra sp. (42.9%) were well represented throughout the stream, whereas another 10 species were found in only one sampling site. Total percentage cover varied from <1% to 90%. Red algae Batrachospermum acuatum and the charophytes Chara vulgaris have the highest percentage cover. Among the parameters analyzed, the stream width, specific conductance and dissolved oxygen were the ones that more closely related to the species number and percentage cover of macroalgal communities. The species number of each site was negatively correlated with dissolved oxygen content. The total percentage cover of the macroalgae was negatively correlated with the stream width and the specific conductance.     

Chemical evolution of the high redshift galaxies

We have tried to determine the rate of chemical evolution of high redshift galaxies from the observed redshift distribution of the heavy element absorption systems in the spectra of QSOs, taking into account the evolution in the intensity of the metagalactic UV ionizing radiation background, the radius and/or the co-moving number density of, and the fraction of mass in the form of gas in, the absorbers. The data for both the Lyman limit systems and the C IV systems have been fitted simultaneously. It seems that the abundance of carbon has possibly increased by about a factor of 5 to 20 from the cosmic time corresponding to the redshift ≃ 4 to 2. The data also suggest that either the radius or the co-moving number density of the galaxies increased with redshift up to z = 2.0 and decreased slowly thereafter. The total mass of the halo gas was higher in the past, almost equal to the entire mass of the galaxy at z = 4. The hydrogen column density distribution for Lyman limit systems predicted by the model is in agreement with the observed distribution.     

A comparison of chemical and chemodynamical models

Representative results from a comparison of the chemical evolution of spherical collapse models without and with a intercloud medium are presented. The hot metal-rich gas distributes quickly the metals produced in supernovae throughout the galaxy, thus leading to a more homogeneous chemical evolution and flatter metallicity gradients in the gas and the stars. The stellar population is somewhat less concentrated towards the centre. The strong outflow results in a substantial loss of metals from the galaxy to its surroundings, and a lower effective yield in the galaxy. This revised version was published online in August 2006 with corrections to the Cover Date.