河南省气象灾害预警信号制作查询系统

河南省气象灾害预警信号制作查询系统是以发布预警信号和查询历吏预警信息为主要目的,通过运用Visual Basic 6．0编程建立预警制作模版,不同强度的预警信号在行政区划地图上以不同颜色区分显示,并可以对河南省历年发布的预警信号基本信息进行入库保存、查询和统计输出：     

径流对区域气候变化的响应研究

利用汾河流域静乐站1970-2004年的气温、降水及径流资料,建立多元非线性回归模型,分析径流变化对区域气候变化的响应,结果表明,径流对降水的响应比气温敏感,且径流变化是气候因子和流域下垫面条件共同作用的结果.     

湖南锡田钨锡多金属矿床流体包裹体显微测温和LA-ICP-MS原位分析对成矿流体演化的制约

为了解锡田钨锡多金属矿床的成矿流体演化过程和成矿元素迁移机制,深入揭示成矿机制,指导该地区的下一步找矿勘探工作,对黑钨矿、锡石及透明矿物的流体包裹体进行了岩相学观察、红外显微测温及LA-ICP-MS原位分析.显示锡田钨锡多金属矿床绿柱石、黑钨矿中发育流体-熔体包裹体,均一温度最高可达760℃.早成矿阶段流体均一温度为360～500℃,盐度主要为28.4%～41.5%Na Cl_eqv,主成矿阶段均一温度为280～450℃,盐度主要为3.0%～20.0%Na Cl_eqv.,晚成矿阶段均一温度为120～280℃,盐度为0.4%～6.6%Na Cl_eqv..LA-ICP-MS分析表明,超临界流体开始出溶时,W、Cu、Mo等元素优先富集于富挥发分气相中,Pb、Zn、Sn、Fe、Mn等元素则更倾向富集于高盐度卤水相中.锡田钨锡多金属矿床成矿流体来源于燕山期浅源花岗岩,钨锡成矿作用始于岩浆-热液过渡阶段,成矿流体具有高温、高盐度和富CO₂等特征.成矿流体来自岩浆流体的出溶,演化过程中经历了两次不混溶作用,不混溶相...     

DIETARY PHOSPHORUS REQUIREMENT OF YOUNG ABALONE, HALIOTIS DISCUS HANNAI INO

An experiment was performed to determine the dietary phosphorus requirement of the young abalone,Haliotis discus hannai. Five semi-purified diets were formulated to provide a series of graded levels of dietary total phosphorus (0.23%–1.98) from monobasic potassium phosphate (KH2P04). The brown alga,Laminaria japonica, was used as a control diet. Similar size abalone were distributed in a single-pass, flow-through system using a completely randomized design with six treatments and three replicates each treatment. The abalone were hand-fed to satiation with appropriate diets in excess, once daily at 17:00. The feeding trial was run for 120-d. Survival rate and soft-body to shell ratio (SB/S) were constantly maintained regardless of dietary treatment. However, the weight gain rate (WGR), daily increment in shell length (DISL), muscle RNA to DNA ratio (RNA/DNA), carcass levels of lipid and protein, soft-body alkaline phosphatase (SBAKP), and phosphorus concentrations of whole body (WB) and soft body (SB) were significantly (ANOVA, P<0.05) affected by the dietary phosphorus level. The dietary phosphorus requirements of the abalone were evaluated from the WGR, DISL, and RNA/DNA ratio respectively, by using second-order polynomial regression analysis. Based on these criteria, about 1.0%–1.2% total dietary phosphorus, i.e. 0.9%–1.1% dietary available phosphorus is recommended for the maximum growth of the abalone. Project 39670572 supported by the NSFC.     

我国土壤中结合态硒的含量和分布规律

本文提出并建立了Jackson法系统分离土壤中不同形态硒的实验程序,研究了我国几种土壤表层(0—20cm)中硒的结合形态及其地理分布规律,并对植物可利用性作了评价。     

Photometry of the contact binary system V471 Cas

UBV photoelectric observations of the W UMa-type binary V471 Cas were made from September to November 1984. Its colour indices were found to be(B-V)=0 _. ^m 771±0 _. ^m 02 and(U-B)=0 _. ^m 196±0 _. ^m 02. TheU, B, andV light curves of V471 Cas show some photometric fluctuations. We found that its orbital period is not 0.335998 days which was given by GCVS (1986), but 0.405356 days.Photometric orbital elements of V471 Cas were found using the Wilson-Devinney method. V471 Cas is a contact system, in which the overcontact factor is 0.19, its mass ratio of two components is 0.5947, and orbital minclination is in 83.29 degrees.     

强磁场下中子星外壳的组分和状态方程

本文计算和讨论了强磁场下由冷的催化物质组成的中子星外壳的组份和状态方程。文中考虑了晶格能和强磁场下均匀电子气体的交换能的贡献.得出结论:(1)强磁场使低密度区的状态方程变软;(2)强磁场对高密度区的状态方程几乎没有影响;(3)核质量公式对外壳的组份影响较明显.     

我国流动SLR首次取得观测成果

介绍了流动SLR系统TROS建成后在北京，乌鲁木齐，拉萨3个站的观测情况。这是流动卫星光测距系统在我国首次正式运行，开创了SLR流动观测的先例，实现了我国SLR领域多年来的愿望。对乌鲁木齐和世界屋脊城市拉萨观测的实现有其重要意义，引起国内外广泛关注。对TROS的建站和观测等问题进行了讨论，给出了观测结果。     

色球活动双星HR1099Hα发射线的高分辨率分光观测和分析

本文给出ＨＲ１０９９（Ｖ７１１Ｔａｕ）的高色散、高分辨率的分光观测结果。从观测结果分析，该双星系统的两子星均有剧烈的色球活动，强的Ｈα发射主峰主要来自活动性强的冷子星，谱线轮廓形状的大幅度变化取决于色球发射物质的运动和恒星内部的物理变化。     

Formation and structure of neutrino astronomical objects

Neutrinos with non-zero mass could gather to form a new kind of astronomical bodies: the Neutrino Astronomical Objects (NAO). We have investigated the mechanism of their formation and the relation of this formation to that of the galaxies, ascertained their e, p, He⁴ content, whose presence should produce a series of observable effects. NAOs are a peculiar kind of heavenly bodies with many new properties. They have a linear size of the order of 100 pc, a total neutrino content of the order of 10¹⁴M and an e, p, He⁴ content of the order of 10⁹M.