综合大洋钻探计划311航次沉积物中自生碳酸盐岩碳、氧稳定同位素特征

为了探索水合物背景下沉积物中自生矿物响应,对采自综合大洋钻探计划（IODP）311航次沉积物中自生碳酸盐岩颗粒进行了矿物组成、形貌特征和碳、氧稳定同位素特征等研究。X光粉晶衍射（XRD）和扫描电镜（SEM）结果显示碳酸盐岩颗粒的主要矿物成分是铁白云石和方解石,呈多孔状结核和不规则状集合体产出。碳酸盐岩颗粒的碳稳定同位素δ¹³C_PDB低至-41.50‰,证实其碳源源自甲烷,其成因与甲烷厌氧氧化过程有关,印证了研究区存在海底甲烷渗漏现象,是甲烷水合物赋存区重要的识别标志之一。碳酸盐岩颗粒的氧稳定同位素δ¹⁸O_PDB总体上随着沉积物深度增加而减小,可能指示沉积物的背景温度由下而上（从早到晚）逐渐降低。研究结果提供了现代海洋天然气水合物背景下沉积物中自生碳酸盐岩的碳、氧稳定同位素记录,对于寻找我国海域天然气水合物资源,探索地史时期古海洋沉积物中类似的甲烷事件记录具有重要的理论和实践指导意义。     

IODP 311航次底栖有孔虫碳稳定同位素对天然气水合物地质系统的指示

为了探索海洋天然气水合物背景下有孔虫特征的响应,对综合大洋钻探计划(IODP) 311航次岩芯沉积物中底栖有孔虫Uvigerina peregrina和Bulimina mexicana进行了初步研究。通过对冷泉站位U1328和毗邻的非冷泉站位U1327沉积物中底栖有孔虫Uvigerina peregrina和Bulimina mexicana的显微形貌特征和碳、氧稳定同位素测试等,证实有孔虫壳体未受到后期成岩作用的改造和自生碳酸盐岩的交代影响,有孔虫壳体的碳稳定同位素呈现明显的负偏。其中U1327站位中U.peregrina δ¹³C为-0.67‰～-2.75‰（PDB）,B.mexicana δ¹³C为-0.51‰～-1.52‰（PDB）;U1328站位中U.peregrina δ¹³C为 -0.72‰～-2.71‰（PDB）,B.mexicanaδ¹³C为 -0.58‰～-1.45‰（PDB）。底栖有孔虫壳体的碳稳定同位素负偏成因可能与水合物不稳定分解释放的甲烷厌氧氧化作用和食物源有关,因而可较好地指示海底天然气水合物系统地质背景。     

沉积物粒度对水合物形成的制约：来自IODP 311航次证据

对取自IODP 311航次（东北太平洋Cascadia大陆边缘）所有5个站位、采样间距约为1.5 m的614件沉积物样品，利用Beckman Coulter LS 230激光粒度仪进行了沉积物粒度分析，获得了沉积物粒度随深度变化特征，进而与水合物层位的替代指标进行了位置对比，这些指标包括特殊沉积构造（soupy和mousse like构造）、测井数据（LWD）推算出来的水合物饱和度（Sh）、岩芯红外图像和实际钻取的含水合物沉积物等。发现沉积物粒度分别为31~63 μm和63~125 μm的2组较粗粒径的沉积物数量变化增多的位置与水合物出现层位之间存在较好的位置对应关系。如在U1326站位海底以下5~8 m、21~26 m、50~123 m、132~140 m、167~180 m、195~206 m、220~240 m深度位置出现了沉积物粒度明显偏向粗粒的趋势，而这些位置正好对应于大多数特殊沉积构造出现的深度，也对应于水合物饱和度（Sh）值相对较高的深度，并与一些实际钻取的赋含水合物的浊积沙层观察结果一致。因此，初步研究后认为，沉积物粒度在水合物形成过程中扮演了重要角色，天然气水合物可能偏向形成于粒度大于31 μm的粗粒沉积物中。       

Predicting demand for 311 non-emergency municipal services: An adaptive space-time kernel approach

Many cities in the United States and Canada offer a 311 helpline to their residents for submitting requests for non-emergency municipal services. By dialing 311, urban residents can report a range of public issues that require governmental attention, including potholes, graffito, sanitation complaints, and tree debris. The demand for these municipal services fluctuates greatly with time and location, which poses multiple challenges to effective deployment of limited resources. To address these challenges, this study uses a locally adaptive space-time kernel approach to model 311 requests as an inhomogeneous Poisson process and presents an analytical framework to generate predictions of 311 demand in space and time. The predictions can be used to optimally allocate resources and staff, reduce response time, and allow long-term dynamic planning. We use a bivariate spatial kernel to identify the spatial structure and weigh each kernel by corresponding past observations to capture the temporal dynamics. Short-term serial dependency and weekly temporality are modeled through the temporal weights, which are adaptive to local community areas. We also transform the computation-intensive parameter estimation procedure to a low dimensional optimization problem by fitting to the autocorrelation function of historical requests. The presented method is demonstrated and validated with sanitation service requests in Chicago. The results indicate that it performs better than common industry practice and conventional spatial models with a comparable computational cost.     

Landslide susceptibility analysis based on citizen reports

Landslide susceptibility estimates are essential for reducing the risk posed by landslides to social and economic well-being. However, estimates of landslide susceptibility depend on reliable landslide inventories whose production requires extensive field or remote sensing efforts. Further, most inventories are not updated through time and thus may not capture the influence of changes in climate and/or land use. Inventories based on citizen reports of landslide occurrence, have the potential to overcome these limitations. Such an inventory can be produced from citizen reports to a 311-phone and online system, a nationwide database that updates real-time and records reported landslides location and timing. Whereas this landslide inventory is promising, it has not used for landslide susceptibility analyses and may be associated with spatial uncertainties and reporting biases. In this study we explore the use of 311-based landslide inventory for landslide susceptibility estimates in Pittsburgh, PA, USA, where landslide risk is among the highest in the nation. We compare the 311-based inventory to field-validated inventories through a multi-pronged approach that combines field validation of 311-reported landslides, probabilistic analysis of the association between landslides and the underlying topographic and geologic factors, and spatial filtering. Our results show that: (a) approximately 70% of the 311-reported landslides are associated with an identifiable landslide in the field; (b) the spatial uncertainty of the 311-reported landslides is 104 ± 25 m; (c) 311-reported landslides differ from other inventories in that they are primarily associated with proximity to roads, however, field-correction of 311-reported landslide locations rectifies this anomaly; (d) a simple spatial filter, scaled by the uncertainty in location as determined from a subset of the 311-data, can increase the consistency between the 311-reported inventory and field-validated inventories. These results suggest that 311-based landslide inventories can improve susceptibility estimates at a relatively low cost and high temporal resolution.     

日本311特大地震地理学报告

应用日本东北地理学会311 地震研究报告资料进行整理完成,系统介绍了这次特大地震的灾情、灾区概况、4 大灾区不同特征、灾害对经济社会的冲击,尤其注重老年少子社会劳动力、汽车主导产业、海洋特色产业、医疗设施和中心城市仙台的影响。     

综合大洋钻探计划311航次沉积物中自生黄铁矿及其硫稳定同位素研究

对综合大洋钻探计划(IODP)311航次652个岩心沉积物样品进行了自生黄铁矿颗粒筛选、显微形貌特征及其硫稳定同位素组成等初步研究。扫描电镜(SEM)照片显示黄铁矿以微球粒状和立方体状形貌产出,其成因与微生物作用和无机作用有关。黄铁矿的δ34SCDT值变化范围较大,从-35.4‰到+53.6‰,其成因与甲烷厌氧氧化作用(AOM)的关系密切。海水源为主的硫酸盐参与了沉积物上部的AOM过程,黄铁矿硫稳定同位素正偏的原因可能与较强的AOM作用和较多的残余硫酸盐参与有关。冷泉背景站位中黄铁矿的δ34SCDT值随着深度增加而增加,从浅表层的-35.83‰增加到深处的32.49‰,反映深处沉积物内黄铁矿形成过程中曾有过较多的残余硫酸盐参与还原,暗示其背景曾经是更高的甲烷通量和更强的AOM作用。研究结果提供了现代海洋天然气水合物背景下沉积物中自生黄铁矿及其硫稳定同位素特征记录,对于寻找我国海域天然气水合物资源,探索地史时期古海洋沉积物中甲烷事件记录具有重要的意义。     

活动小行星311P/PANSTARRS的动力学lk 特性分析

311P/PANSTARRS是一颗活动小行星, 具有小行星和彗星的双重特征, 是中国``天问二号''的探测目标之一. 311P/PANSTARRS直径较小, 约为400 m, 非引力效应可能会对其长期动力学演化产生较大的影响. 通过假定不同表面组分, 研究了Yarkovsky效应对311P/PANSTARRS轨道演化的影响, 讨论了密近交汇、 非破坏性碰撞和YORP (Yarkovsky-O''Keefe-Radzievskii-Paddack)效应等非引力效应, 计算了小行星与大行星密近交汇及碰撞概率, 估计了311P/PANSTARRS达到自转周期分裂极限的时标. 模拟结果显示与纯引力模型相比, Yarkovsky效应可能会加快311P/PANSTARRS离开当前共振区域, 大约在10Myr以后311P/PANSTARRS会离开当前所在共振带, 在表面覆盖风化层的情况下有机会通过v6长期共振成为越火小行星; 在考虑YORP效应的情况下, 311P/PANSTARRS在2 Myr时标内可达到自转周期分裂极限; 在考虑Yarkovsky效应及YORP效应等因素的情况下, 311P/PANSTARRS在10 Myr时标内仍可保持其动力学稳定性, 且YORP效应不会显著影响其半长径偏移量.     

IODP 311航次底栖有孔虫碳稳定同位素对天然气水合物地质系统的指示

为了探索海洋天然气水合物背景下有孔虫特征的响应,对综合大洋钻探计划(IODP)311航次岩芯沉积物中底栖有孔虫Uvigerina peregrina和Bulimina mexicana进行了初步研究。通过对冷泉站位U1328和毗邻的非冷泉站位U1327沉积物中底栖有孔虫Uvigerina peregrina和Buliminamexicana的显微形貌特征和碳、氧稳定同位素测试等,证实有孔虫壳体未受到后期成岩作用的改造和自生碳酸盐岩的交代影响,有孔虫壳体的碳稳定同位素呈现明显的负偏。其中U1327站位中U.peregrinaδ13C为-0.67‰~-2.75‰(PDB),B.mexicanaδ13C为-0.51‰~-1.52‰(PDB);U1328站位中U.peregrinaδ13C为-0.72‰~-2.71‰(PDB),B.mexicanaδ13C为-0.58‰~-1.45‰(PDB)。底栖有孔虫壳体的碳稳定同位素负偏成因可能与水合物不稳定分解释放的甲烷厌氧氧化作用和食物源有关,因而可较好地指示海底天然气水合物系统地质背景。     

Deep echelle spectrophotometry of S 311, a Galactic H ii region located outside the solar circle

We present echelle spectrophotometry of the Galactic H  ii region S 311. The data have been taken with the Very Large Telescope Ultraviolet-Visual Echelle Spectrograph in the 3100–10 400 Å range. We have measured the intensities of 263 emission lines; 178 are permitted lines of H⁰, D⁰ (deuterium), He⁰, C⁰, C⁺, N⁰, N⁺, O⁰, O⁺, S⁺, Si⁰, Si⁺, Ar⁰ and Fe⁰; some of them are produced by recombination and others mainly by fluorescence. Physical conditions have been derived using different continuum- and line-intensity ratios. We have derived He⁺, C⁺⁺ and O⁺⁺ ionic abundances from pure recombination lines as well as abundances from collisionally excited lines for a large number of ions of different elements. We have obtained consistent estimations of t ² applying different methods. We have found that the temperature fluctuations paradigm is consistent with the T _e(He  i ) versus T _e(H  i ) relation for H  ii regions, in contrast with what has been found for planetary nebulae. We report the detection of deuterium Balmer lines up to Dδ in the blue wings of the hydrogen lines, whose excitation mechanism seems to be continuum fluorescence.