赤道几内亚里奥穆尼盆地石油地质特征及勘探方向

位于赤道几内亚的里奥穆尼盆地是裂谷盆地与被动大陆边缘盆地叠加的中-新生代复合型含油气盆地.盆地的构造演化经历了裂谷期、过渡期和漂移期三个阶段.盆地地层以过渡期盐岩层为界,盐下为裂谷期层序,盐上为漂移期层序.盆地生储盖组合可以划分为上、中、下三套,中组合最为有利.盐下裂谷期圈闭类型以断块圈闭和背斜圈闭为主,盐上漂移期以盐...     

雪龙在线网络信息平台的研发与展望

雪龙在线是一个连接"雪龙"号与国内的网络信息平台,借助于海事卫星通讯链路(BGAN)将船上航行动态信息与科考仪器数据与国内服务器进行交换,并在互联网实时发布获取的动态数据,为极地考察主管部门、考察队员及其家属以及社会公众提供一个了解"雪龙"号航行状态、关注极地考察的窗口,并可通过国内专家团队和专业数据产品为"雪龙"号航...     

基于GPS的“雪龙”船冲击式破冰模式识别研究

"雪龙"号破冰船是我国目前唯一的极地考察船,破冰航行是极地船舶的重要特征之一。以"雪龙"号破冰船的GPS数据为基础,通过建立模型算法识别冲击式破冰这一特殊的航行状态,在整个中国第28次南极考察航次的数据分析中,整体识别率超过86.1%,识别正确率达到98%以上。利用此算法,在中国第27次南极考察航次的破冰识别率也超过85%,识别正确率达到93.5%。雪龙船两个航次实测GPS数据验证了本文算法的可用性,而破冰识别统计结果表明,不同航次的破冰模式具有较大的差异。     

中国极地考察站广域网通信建设与服务现状及展望

通过中国极地考察"十五"能力南极两站卫星通信网络系统项目的建设,我国南极考察站的广域网通信能力和站区网络通信能力已经有了很大提高。系统阐述南极两站的广域网通信现状,内容包括南极两站卫星通信链路的建设情况、考察站计算机网络系统建设情况以及该系统所提供的服务情况,涉及卫星通信、局域网以及VOIP等技术;对未来几年极地考察通信中可能会采用的通信技术建设提出建议。     

南极中山站至Dome A剖面表面雪样氧同位素组成

运用质谱技术 ,测定了南极中山站至 Dome A剖面 1 998/1 999年度表面雪样氧同位素组成。结果表明 ,表面雪样氧同位素组成变化范围相当大 (- 2 2 .5 1‰ - - 5 0 .6 7‰ ) ,且具有随距中山站距离逐渐增大、海拔高度逐渐增加而逐渐减小的趋势。线性回归分析显示表面雪样氧同位素组成与距中山站距离、海拔高度和纬度存在着很好的相关性 ,这实际上反映出稳定同位素组成和温度之间的密切联系     

唐山M4.8级和宝坻M4.0级地震前的地电场异常变化

以2012年5月28日唐山M4．8级地震和6月18日天津市宝坻区M4．0级地震为研究对象,利用天津宝坻、静海及徐庄子地震台ZD9A大地电场仪的观测资料,使用地电场观测的同一测向长、短极距测值的比值法进行分钟值数据处理,结果表明地震前这3个台站地电场观测资料有不同程度的短临异常变化。     

孟加拉扇更新统加积型深水水道规模和演化

近年来,深水油气勘探发现的储量在全球新增储量中的占比逐年增加,2010年以来其占比已超过50%,深水已经成为未来油气勘探的重点领域。作为深水油气勘探主要储层之一的深水水道,同样成为深水油气勘探的重点研究对象。以高分辨率（40 Hz）三维地震资料为基础,对研究区内的加积型水道—天然堤复合体进行了精细刻画,着重刻画了水道—天然堤复合体内部不同期次水道的中心线,重点分析了深水水道的发育和演化特征。该水道天然堤复合体整体宽25～30 km,单期水道宽度约300 m,推测厚度约10 m。深水水道的演化整体表现为有序的发育过程,初期水道较顺直,弯曲度较低,后期弯曲度逐渐升高,晚期水道的平面形态较为稳定,变化较小。深水水道在演化过程中不仅向左右两侧迁移,同时也具有向下游方向迁移的特征;前人认为深水水道向下游迁移的现象非常罕见,但是研究表明在某些情况下,这种现象可能并不罕见。     

A Space‐Time Raster GIS Data Model for Spatiotemporal Analysis of Vegetation Responses to a Freeze Event

Many past space‐time GIS data models viewed the world mainly from a spatial perspective. They attached a time stamp to each state of an entity or the entire area of study. This approach is less efficient for certain spatio‐temporal analyses that focus on how locations change over time, which require researchers to view each location from a temporal perspective. In this article, we present a data model to organize multi‐temporal remote sensing datasets and track their changes at the individual pixel level. This data model can also integrate raster datasets from heterogeneous sources under a unified framework. The proposed data model consists of several object classes under a hierarchical structure. Each object class is associated with specific properties and behaviors to facilitate efficient spatio‐temporal analyses. We apply this data model to a case study of analyzing the impact of the 2007 freeze in Knoxville, Tennessee. The characteristics of different vegetation clusters before, during, and after the 2007 freeze event are compared. Our findings indicate that the majority of the study area is impacted by this freeze event, and different vegetation types show different response patterns to this freeze.     

The effect of the equatorially symmetric zonal winds of Saturn on its gravitational field

The penetration depth of Saturn’s cloud-level winds into its interior is unknown.A possible way of estimating the depth is through measurement of the effect of the winds on the planet’s gravitational field.We use a self-consistent perturbation approach to study how the equatorially symmetric zonal winds of Saturn contribute to its gravitational field.An important advantage of this approach is that the variation of its gravitational field solely caused by the winds can be isolated and identified because the leading-order problem accounts exactly for rotational distortion,thereby determining the irregular shape and internal structure of the hydrostatic Saturn.We assume that(i)the zonal winds are maintained by thermal convection in the form of non-axisymmetric columnar rolls and(ii)the internal structure of the winds,because of the Taylor-Proundman theorem,can be uniquely determined by the observed cloud-level winds.We calculate both the variation △J_n,n=2,4,6...of the axisymmetric gravitational coefficients J_n caused by the zonal winds and the non-axisymmetric gravitational coefficients △J_(nm) produced by the columnar rolls,where m is the azimuthal wavenumber of the rolls.We consider three different cases characterized by the penetration depth 0.36 R_S,0.2 R_S and 0.1 R_S,where R_S is the equatorial radius of Saturn at the 1-bar pressure level.We find that the high-degree gravitational coefficient ( J_(12)+△J_(12)) is dominated,in all the three cases,by the effect of the zonal flow with |△J_(12)/J_(12)|100%and that the size of the non-axisymmetric coefficientsdirectly reflects the depth and scale of the flow taking place in the Saturnian interior.     

弧板式透空堤消浪性能影响因素数值研究

弧板式透空堤是由弧型板组成的新型防波堤结构。为探讨其透射系数的影响因素,利用Fluent软件基于N-S方程构建了波浪与板式透空堤相互作用的数值模型,讨论了相对潜深、入射波周期、相对波高、相对板宽和结构型式对透射系数的影响。结果表明:弧板式透空堤的透射系数随着相对波高和入射波周期的增大而增大,在静水面附近透射系数最小,尤以静水面和略高于静水面时的消浪效果最佳;在相同波浪要素条件下,静水面及其上0.02 m和0.04 m位置处,弧板式透空堤的消浪效果明显优于平板式透空堤。