立波作用下的底沙运动

立波作用下的底沙运动关系到港口的规划和建筑物的安全。本文以实验为基础，综合前人研究成果，得到立波作用下床面形态及冲刷类型。对较粗颗粒底沙在立波作用上进行受力分析，得到了一周期内沙粒累计推移距离，净输沙率及冲刷强度。认为冲刷形态的不同与近底速度和加速度的分布密切相连。     

南汇近岸水域近底层泥沙运动和边滩沉积

根据长江口南汇近岸水域17个站的水文泥沙同步观测资料,阐述了该水域近底层泥沙的流速、悬沙浓度的分布和变化。经无量纲潮流动力值的计算表明,研究区存在一个包络南汇边滩先向东南继而向南延伸的舌状高能量区,与高悬沙浓度分布区相一致。通过对悬沙运动和涨、落潮周期流向的分析,揭示了长江口向杭州湾底层泥沙输移的规律,其底层泥沙输移主要集中在低潮位时段,输移时间约占潮周期的36%,其中以南汇边滩向杭州湾输移的时间为最长,大、小潮都在5h以上,与其相关联,在芦潮港水域下层存在着一股东西向的高悬沙浓度的水体。据盐度、潮流、悬沙浓度等要素,并结合絮凝沉降分析得出,南汇边滩的沉积强度是潮滩>潮下带>深水区;边滩舌尖前缘水域的泥沙沉积时间与水体出现向东偏南或向西流的时间一致,这可视为近年来南汇水下沙嘴向东偏南伸展的原因之一。     

广西近海海水溶质稀释扩散现场实验与COD潮扩散数值模拟

海水的稀释扩散是一个十分复杂的问题.在近岸海域,弯曲的海岸线、不同的水深、变化的天气、随机的海浪和周期性的潮汐潮流都对海水的扩散产生直接影响.Joseph和Sendner[1],Okubo[2],及国内的张法高[3]、李培泉[4]、周家义[5]、姜太良[6]等进行了现场实验或数值方面的研究.1992～1996年,我们对广西近海海洋环境进行了8个航次的综合调查,并在广西廉州湾和铁山港进行了数次海水稀释扩散现场实验.     

沿海深水岸段排污口近区污染物混合过程的模拟方法

本文提出一种将二维动态水质模型与三维稳态水质模型有机结合的新方法，用来处理沿海深水岸段排污口近区污染物混合问题，使之能较好地再现其客观混合过程。将这种方法应用于深圳大鹏湾某大型石化项目的环境影响预测中．结果令人满意。     

Electromagnetic Subsurface Imaging. A Case for an Adaptive Born Approximation

The process of interpretation of electromagnetic data has many facets of which fast approximate interpretation techniques is an intriguing one. A new variant of the Born approximation – the Adaptive Born approximation – is presented and exemplified through 1D and 2D imaging techniques for transient electromagnetic data. The Adaptive Born approximation is generally applicable in approximate inversion schemes for inductive electromagnetic data as a one-pass imaging algorithm. Though it is as simple to use as the ordinary Born approximation, it offers a more accurate inverse mapping.In the first part of this paper an attempt will be made to give an overview of fundamental concepts in electromagnetic subsurface imaging relevant for approximate inverse mappings and to outline major trends in present day modeling and inversion of electromagnetic data. This is of course an impossible task – certainly for this author – and much important work will not be mentioned in the limited space of the following. My apologies to the people who are not mentioned and whose research is not given credit here though it should have been. Naturally, my choice of references reflects the schools and circles I have been subjected to, but I hope that the list of references to developments in electromagnetic methods will point to papers of importance and thereby to other references for the interested reader.     

3—D叠前成像速度分析

“深度成像”是近年来使复杂的构造地震成像发生深刻变化最具决定意义的技术。与常规时间成像相比,深度成像明显的优点是揭示了盐下构造的形态和提高了成像的清晰度。本文将重温偏移成像的基本原理,并着重论述了一种用于层速度分析的稳健技术－用３－Ｄ叠前深度成像估算层速度和反射层位置。     

Circumstellar molecular line absorption and emission in the optical spectra of post-AGB stars

We present preliminary results obtained with the European Observation Network. This network consists of 9 observatories in the Czech Republic, Germany and Bulgaria and has been involved in the BACODINE activities since April 1, 1994. We also discuss related problems such as the background of unknown variable stars and suggest a strategy for work in this area.     

A deeply embedded companion to LKHα198

The region around the Herbig Ae/Be star LkH198 was imaged at 10m with the CAMIRAS camera at the Canada-France-Hawaii Telescope and the Nordic Optical Telescope. We discovered a deeply embedded companion 6 north of LkH198, which may be responsible for most of the far-infrared emission in the region and for driving the molecular flow. LkH198 appears point-like at our resolution (FWHM 1.3), excluding an extended envelope of transiently heated small grains as the dominant origin of the mid-infrared excess in that star.     

Development of the hard X-ray imaging experiment timax: Laboratory images and first balloon flight

We present calibration results and laboratory images produced by the balloon-borne hard X-ray imaging telescope TIMAX. The images were produced with an²⁴¹Am radioactive source placed 45 m away from the detector plane, in the center of the field of view. It is shown that the mask 3-antimask imaging reconstruction process, when combined with flat-fielding techniques, is very effective at recovering signal-to-noise ratio lost due to systematic non-uniformity in the background measured by the 35 detectors. The experiment was launched in June 8th, 1993 from Birigüi, SP, Brazil, onboard a 186,000 m³ stratospheric balloon, and remained at an atmospheric depth of 2 g cm^–2su for 8 hours. Even though no scientific data were gathered in this first flight, we obtained valuable engineering data and could also calculate the sensitivity of the experiment based on the instrumental background spectrum at balloon altitudes. In the 60–70 keV energy band, the experiment can detect 3 sources at a level of 1.2 x 10^–4 photons cm^–2 s^–1 keV^–1 for an integration of 6 hours at 2.1 g cm^–2.