Effect of dietary protein to energy ratio on growth and nitrogenous waste production of cultured dusky kob Argyrosomus japonicus

The effect of dietary protein to energy ratio (P:E) on the growth of dusky kob Argyrosomus japoni-cus was investigated as a first step towards formulating a practical diet for this potential mariculture species in South Africa. The effects of dietary protein and lipid on growth, feed conversion ratio (FCR) and nitrogenous waste production were determined in cultured juveniles (initial weight 113.8 ± 2.0 g fish^?1). Fish were fed diets that contained either 42 or 46% protein with 6, 12 or 18% lipid, within a P:E range of 20.5–26.7 g protein MJ^?1. Weight gain and specific growth rate (SGR) were significantly influenced by an interaction between dietary protein and energy (p < 0.001). An increase in dietary lipid produced increasing growth rates (ranging from 0.95 ± 0.04% to 1.10 ± 0.01% day^?1) among fish fed the 46% protein diets, with no significant differences in FCR (1.05 ± 0.02 to 1.11 ± 0.02) or protein efficiency ratio (PER; 1.95 ± 0.06 to 1.66 ± 0.02). By contrast, there was a trend of decreasing growth (0.96 ± 0.04% to 0.64 ± 0.03% day^?1) and a deterioration in FCR (1.3 ± 0.10 to 1.93 ± 0.19) and PER (1.12 ± 0.11 to 1.68 ± 0.11) with increasing dietary lipid among fish fed 42% protein diets, indicating a protein– energy imbalance. The protein and lipid levels tested here had no significant effect on total ammonia production, with a combined mean production of 2.54 ± 0.55 mg kg^?1 I^?1 h^?1, 10 hours postprandial (p = 0.68). The dietary lipid level appeared to directly determine the carcass lipid content, with the mean lipid content ranging from 4.2% to 17.8% for fish fed diets ranging from 6% to 18% respectively after 12 weeks (r² = 0.98). A 46% protein and 18% lipid (P:E ratio of 22.0 g protein MJ^?1) diet is recommended for rearing juvenile A. japonicus of a mass range of 100–300 g.     

热压高磷铁基胎体性能及其金刚石钻头研究

针对在硬而致密岩石中钻进时效低和钻头使用寿命短以及传统金刚石钻头胎体材料价格高等众多难题,采用混料回归试验设计方法,进行了替代碳化钨基金刚石钻头胎体材料的新型铁基胎体配方的试验研究;分析了热压钻头的金刚石出刃与岩石研磨性等岩性之间的内在联系,认为钻头的胎体成分及其性能是关键。因此,从热压金刚石钻头的胎体成分与性能研究入手,经过反复的试验研究与优化组合,研究出热压高磷铁基孕镶金刚石钻头的胎体材料,并试制出金刚石钻头。在室内对可钻性Ⅸ级岩石进行钻进的试验表明：钻进时效平均达到1．91m,钻头平均工作寿命达到60．26m。试验结果表明,高磷铁基眙体是一种性能良好的金刚石钻头胎体材料,且该类型胎体的热压金刚石钻头是一种成本明显降低、具有广谱性能的金刚石钻头。     

Post-cropping change and dynamics in soil and vegetation properties after forest clearing: Example of the semi-arid Mikea Region (southwestern Madagascar)

This study concerns post-cultural dynamics in the semi-arid South-West of Madagascar (Analabo area, near the Mikea Forest). A synchronic comparison was performed on a set of abandoned fields plots aged from 2 to 30 years and on forest and savanna reference ecosystems, located on cambic arenosols developed from same Quaternary dune sands. The studied parameters concerned mainly a few physical and chemical soil properties (density, permeability, compaction, texture, C, N, K, P content). Important changes occur in the post-cultural succession: an increase of the soil density and compaction, and decrease of the soil upper layer permeability. Consequently, slash and burn cultivation leads to a packing and an induration of the soil surface. Results about edaphic indicators have shown that the physical parameters used better discriminate various stages of evolution than the chemical parameters do. The multivariate analysis of soil indicators shows that vegetative succession over 30 years in a forest ecosystem cleared, burnt, cultivated and left, does not lead to features corresponding to a closed-canopy forest but rather to those of a tree savanna with open, mixed woody-herbaceous vegetation. The primary dense dry deciduous regeneration of the primary forest is very low or nil. In the semi-arid SW Madagascar (Analabo region), post-cultural dynamics conditions consists in a savanna-formation process, controlled by: (1) the intensity and duration of the disturbance (during the cultivation phase); and (2) the more drastic environmental conditions (including both climate and soil).     

GPS双频接收机C/A码与P码伪距精度的分析和比较

本文主要研究GPS双频接收机C/A码和P码伪距的精度问题,首先阐述了保密P(Y)码伪距的测量原理,然后采用自行编制的精密单点定位程序,利用大量IGS跟踪站观测数据进行了试算,对该问题进行了探讨和分析,结论认为C/A码和P1码伪距的精度基本相同,而P2码伪距观测值的精度较低。     

Pollution characteristics of polycyclic aromatic hydrocarbons （PAHs） in oily sludge from the Zhongyuan Oilfield and its peripheral soils

The purpose of this study is to determine the degree of contamination caused by polycyclic aromatic hydrocarbons (PAHs) in oily sludge and soils around it in the Zhongyuan Oilfield. The contents of polycyclic aromatic hydrocarbons in oily sludge samples were determined with HPLC. The contents of PAHs of oily sludge from three different oil production plants vary from high to low in the order of the Wenming oily sludge dumping site of No. 3 Oil Production Plant (3W)>the Mazhai oily sludge dumping site of No. 3 Oil Production Plant (3M)>the Wen’er oily sludge dumping site of No. 4 Oil Production Plant (4W). Naphthalene, acenaphthylene, acenaphthene, fluorine and phenanthrene are the major pollutants of PAHs in oily sludge. The contents of PAHs in soil samples around the oily sludge dumping sites vary widely from 434.49 to 2408.8 ng/g. Naphthalene, acenaphthene, fluorine, phenanthrene and pyrene are the characteristic factors of PAHs in soil samples of 3M and 3W, and naphthalene, acenaphthene, fluorine and phenanthrene are the characteristic factors of PAHs in soil samples of 4W. According to these data and the ratios of Fl/Py, PAHs in oily sludge samples come mainly from petrogenic sources, and soil samples are divided into petrogenic soil samples and mixed-source soil samples, and both petrogenic and pyrogenic soil samples in terms of the sources of PAHs. The classification by Nemero index P indicates that soils around the oily sludge dumping sites have been seriously polluted.     

Raw mix designing, clinkerization and manufacturing of high-strength Portland cement from the limestone and clay of Darukhula Nizampur, Nowshera District, North-West Frontier Province （N.W.F.P.）, Pakistan

This paper covers the detailed version of the potential raw material deposits at Darukhula and the adjacent areas of Nizampur, the manufacturing of high-strength Portland cement samples from the same material and comparison of the physical and chemical parameters for resulting cement with British and Pakistan standard specifications, which include compressive strength, setting time, consistency, lechatelier expansion, Blaine and insoluble residue. It was found that the raw material available in the study area meets the standard specifications and the area is feasible for the cement plant installation. The area can provide raw material which is quite sufficient for the running of a cement plant.     

大别山朱家冲高压榴辉岩变质演化特征分析

研究表明大别山朱家冲榴辉岩属于典型的高压榴辉岩,其具有复杂的变质演化历史。根据岩相学、矿物成份化学和热力学分析表明,该类榴辉岩记录了6期变质过程,具有“顺时针”的P?T演化轨迹。由Ⅰ?阶段、Ⅱ?阶段至Ⅲ?阶段显示了近于等温增压进变质特征,并在 Ⅲ?阶段压力值最高达到P＝2.53 GPa; Ⅳ?阶段和Ⅴ?阶段则表现为增温降压退变过程,温度在 Ⅴ?阶段最高达到T＝627 ℃; 到Ⅵ?阶段则为降温降压过程。该过程暗示了高压板片在俯冲和折返过程中可能处于一个非匀速的状态。推测朱家冲榴辉岩后期增温退变的过程可能是源于受扰动的地温线恢复、超高压榴辉岩退变过程的“散热”以及该类榴辉岩对温度变化极为敏感所致。     

Large cometary grains – their destruction and changes in the luminosity of comets

The catastrophic thermodynamic destruction of large cometary heterogeneous grains lying on the surface of a comet nucleus is examined. The core–mantle grain-structure model is assumed. Grain fragmentation as an explanation of sudden changes in cometary brightness is proposed. The approach presented to the problem of cometary outbursts is a development of a previous author's paper. The proposed mechanism is based on the idea of thermodynamical destruction of heterogeneous cometary grains. Numerical simulations have been carried out for a wide range of values of physical characteristics of cometary material. The results obtained are consistent with observational data. The main conclusion of this paper is that thermodynamical fragmentation of large grains can explain variations in brightness and also outbursts of comets.     

A revisit to agglomerates of early‐type Hipparcos stars

We study the spatial structure and sub‐structure of regions rich in Hipparcos stars with blue B_T – V_T colours. These regions, which comprise large stellar complexes, OB associations, and young open clusters, are tracers of on‐going star formation in the Galaxy. The DBSCAN (Density‐Based Spatial Clustering of Applications with Noise) data clustering algorithm is used to look for spatial overdensities of early‐type stars. Once an overdensity, “agglomerate”, is identified, we carry out a data and bibliographic compilation of their star member candidates. The actual membership in agglomerate of each early‐type star is studied based on its heliocentric distance, proper motion, and previous spectro‐photometric information. We identify 35 agglomerates of early‐type Hipparcos stars. Most of them are associated to previously known clusters and OB associations. The previously unknown P Puppis agglomerate is subject of a dedicated study with Virtual Observatory tools. It is actually a new, nearby, young open cluster (d ∼ 470 pc, age ∼ 20 Ma) with a clear radial density gradient.We list P Puppis and other six agglomerates (including NGC 2451 A, vdBH 23, and Trumpler 10) as new sites for substellar searches because of their youth, closeness, and spatial density. We investigate in detail the sub‐structure in the Orion, CMa‐Pup and Pup‐Vel OB complexes (“super‐agglomerates”). We confirm or discover some stellar overdensities in the Orion complex, like the 25 Ori group, the Horsehead region (including the σ Orionis cluster), and the η Orionis agglomerate. Finally, we derive accurate parallactic distances to the Pleiades, NGC 2451 A, and IC 2391, describe several field early‐type stars at d < 200 pc, and discuss the incompleteness of our search. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)