Time variability of Martian bolometric albedo

A time-sequential set of bolometric albedo maps for Mars has been constructed from Viking Infrared Thermal Mapper data. The maps provide global coverage in longitude for latitudes -60° to +60° at 1° by 1° spatial resolution. Individual maps are constructed under strict geometric constraints for a narrow range of L_s. The set of albedo maps spans a Martian year and includes maps before, during, and after the global dust storms of 1977. Transient brightenings associated with local dust storms or condensate clouds are apparent in some of the maps. During dust-free periods, bolometric albedo maps are generally similar to classical, visual albedo map of Mars. The distribution of bolometric surface albedos is bimodal with typical, clear-sky, Lambert albedos of 0.27 and 0.16 for bright and dark areas, respectively. Atmospheric effects strongly influence apparent surface albedos, especially for dark areas. Neither bright nor dark regions show measurable, long-term variations of bolometric albedos during clear periods.     

Numerical simulation of the final stages of terrestrial planet formation

Three representative numerical simulations of the growth of the terrestrial planets by accretion of large protoplanets are presented. The mass and relative-velocity distributions of the bodies in these simulations are free to evolve simultaneously in response to close gravitational encounters and occasional collisions between bodies. The collisions between bodies, therefore, arise in a natural way and the assumption of expressions for the relative velocity distribution and the gravitational collision cross section is unnecessary. These simulations indicate that the growth of bodies with final masses approaching those of Venus and the Earth is possible, at least for the case of a two-dimensional system. Simulations assuming an initial uniform distribution of orbital eccentricities on the interval from 0 to e_max are found to produce final states containing too many bodies with masses which are too small when e_max < 0.10, while simulations with e_max > 0.20 result in too many catastrophic collisions between bodies thus preventing rapid accretion of planetary-size bodies. The e_max = 0.15 simulation ends with a state surprisingly similar to that of the present terrestrial planets and, therefore, provides a rough estimate of the range of radial sampling to be expected for the terrestrial planets.     

雌雄比对海带雌配子体发育的影响

本实验进行了不同雌雄比对海带雌配子体发育的影响。结果表明：雌雄比(鲜重)为1：1及2：1，实验组出现排卵时间最早，且发育率高，实验第20天，发育率超过70％，孢子体正常。5：1，10：1，20：1实验组随着雄性比例的减少，发育率逐渐降低，随着培养天数的增加，三个实验组均出现未受精卵及畸形孢子体，雌雄比越大，未受精卵数目越多。     

Coming to the table: Early stakeholder engagement in marine spatial planning

From 2009 to 2011, marine spatial planning (MSP) rapidly gained visibility in the United States as a promising ocean management tool. A few small-scale planning efforts were completed in state waters, and the Obama Administration proposed a framework for large-scale regional MSP throughout the U.S. Exclusive Economic Zone. During that same time period, the authors engaged a variety of U.S ocean stakeholders in a series of dialogs with several goals: to share information about what MSP is or could be, to hear stakeholder views and concerns about MSP, and to foster better understanding between those who depend on ocean resources for their livelihood and ocean conservation advocates. The stakeholder meetings were supplemented with several rounds of in-depth interviews and a survey. Despite some predictable areas of conflict, project participants agreed on a number of issues related to stakeholder engagement in MSP: all felt strongly that government planners need to engage outsiders earlier, more often, more meaningfully, and through an open and transparent process. Equally important, the project affirmed the value of bringing unlike parties together at the earliest opportunity to learn, talk, and listen to others with whom they rarely engage.     

A review of marine mammal,sea turtle and seabird bycatch in USA fisheries and the role of policy in shaping management

This paper reviews the available information (observer programs, estimates, statutes, regulations) for bycatch of marine mammals, sea turtles, and seabirds in fisheries of the United States. Goals of the review were to evaluate the state of knowledge of bycatch and the role of existing protective legislation in shaping bycatch management for different taxa. Pressing issues are identified, as well as knowledge gaps and policy limitations that hinder multi-species bycatch reduction. The USA has made important progress toward reducing bycatch in its fisheries, but the efficacy of its management has been limited somewhat by a focus on taxon- and fishery-specific regulation and the lack of consistent mandate across taxa for taking a cumulative perspective on bycatch. Applying consistent criteria across taxa for setting bycatch limits (e.g., extending the approach used for marine mammals to sea turtles and seabirds) would be the first step in a multi-species approach to bycatch reduction. A population-based multi-species multi-gear approach to bycatch would help identify priority areas where resources are needed most and can be used most effectively.     

辽东湾中部海域春季大型底栖生物的群落结构及影响因子

2013年5月对辽东湾中部的大型底栖生物进行了调查,分析了该海域底栖生物的种类组成、丰度、生物量、群落结构及其与环境因子的关系。调查海域共发现大型底栖生物70种,包括多毛类24种,甲壳类18种,软体动物20种,棘皮动物7种,纽虫1种。相对重要性指数大于100的种类有14种,排名前3位的分别是日本游泳水虱、毛蚶、日本长尾虫。底栖动物丰度平均值为244.2个/m~2,生物量为52.52 g/m~2,棘皮动物是生物量的重要贡献者。多样性指数平均值为3.24,丰度生物量比较曲线分析结果认为调查海域大型底栖动物群落未受到干扰,底栖生物群落的结构相似性较低,在20%的相似程度上可分为5个组。底层水中溶解氧含量是影响底栖生物的主要因素,不同底质条件是影响底栖生物生物量和群落结构的重要因素。     

Remote estimation of surficial seafloor properties through the application Angular Range Analysis to multibeam sonar data

The variation of the backscatter strength with the angle of incidence is an intrinsic property of the seafloor, which can be used in methods for acoustic seafloor characterization. Although multibeam sonars acquire backscatter over a wide range of incidence angles, the angular information is normally neglected during standard backscatter processing and mosaicking. An approach called Angular Range Analysis has been developed to preserve the backscatter angular information, and use it for remote estimation of seafloor properties. Angular Range Analysis starts with the beam-by-beam time-series of acoustic backscatter provided by the multibeam sonar and then corrects the backscatter for seafloor slope, beam pattern, time varying and angle varying gains, and area of insonification. Subsequently a series of parameters are calculated from the stacking of consecutive time series over a spatial scale that approximates half of the swath width. Based on these calculated parameters and the inversion of an acoustic backscatter model, we estimate the acoustic impedance and the roughness of the insonified area on the seafloor. In the process of this inversion, the behavior of the model parameters is constrained by established inter-property relationships. The approach has been tested using a 300 kHz Simrad EM3000 multibeam sonar in Little Bay, NH. Impedance estimates are compared to in situ measurements of sound speed. The comparison shows a very good correlation, indicating the potential of this approach for robust seafloor characterization.     

胜利海上油田分队计量研究

通过γ射线穿透油、气、水混合物后的透射和散射计数,经理论模拟计算,实现对原油含水率在线计量分析,测量含水率范围为３％－１００％,精度在２％以内。在实际应用过程中,运行稳定,易于操作,特别是修正了由于原油中含气地含水率测量带来的误差,技术和性能指标均已契过以往各种含水测量仪,通过应用,实现了海洋石油开发公司采油一、二分公司和油气集输大队的分队计量,使生产管理水平整体上了一个新台阶。     

半封闭海湾固有振动周期的数值计算

用二维数值模式,根据芝罘湾的实测水深和形状,计算了该湾的固有振动周期,与实测资料吻合较好。计算结果同时给出了当节点N=1,2,...,6时,湾内的振幅分布（合波长、波节线分布）,以及纵振动和横振动分布情况。     

基于X射线连续谱的光子计数探测器能量标定方法

随着探测器技术的发展,具有能量分辨能力的光子计数探测器在X射线能谱CT成像中应用越来越广泛。能量与阈值的对应关系对能谱CT成像具有重要意义,受到实验条件的限制,目前的光子计数探测器的能量标定方法有一定的局限性。针对光子计数探测器的单像素标定问题,本文提出一种基于X射线光机连续谱的能量标定方法,通过建立和分析X光谱模型,利用光机连续谱中高能端的能量信息,得到阈值与能量之间的关系。实验结果表明该方法操作方便,对探测器单像素标定结果较为准确,对其他类型光子计数探测器的标定具有参考意义。