海水溶解氧自动电位滴定分析方法研究

本项研究直接采用ZDJ-4A型自动电位滴定仪及其铂金-甘汞电极体系测定海水中的溶解氧,具有操作简单、稳定可靠、速度快、精度高和适于现场使用等优点.大量实验数据表明,该分析方法的测量精密度和重复性精密度已达优于士0.02mg/l之水平,测量准确度与经典的温克勒法持平,基本实现了海水溶解氧的自动化分析.     

HJ-1B 热红外波段在轨绝对辐射定标

针对HJ-1B 红外相机(IRS)热红外通道特点, 利用青海湖辐射校正场进行HJ-1B 热红外绝对辐射定标, 提 出新的场地定标算法, 并通过实测数据和Landsat5-TM数据对不同定标系数进行真实性检验分析, 发现该场地定标 算法获得的系数比原始系数精度提高约0.6%—3%, 总体精度为1K 左右。研究结果表明文章提出的定标算法适用 于不具备观测冷空间能力的卫星传感器在轨绝对辐射定标, 得到的定标系数合理可靠。     

1:10 000 DLG交通核心要素快速更新的卫星影像数据源的比较与选择

对1∶10 000 DLG交通核心要素快速更新的卫星数据源进行比较和分析,主要是分辨率为2.5 m的ALOS,SPOT5和2.36 m的中巴02B卫星影像。从数据质量、校正精度、重访时间及价格对它们进行了分析与比较,综合这些因素认为三者中ALOS是目前最佳数据源,SPOT5可作为数据补充,而02B影像由于校正精度较差不能选用。     

CLASS B2108+213: a new wide-separation gravitational lens system

We present observations of CLASS B2108+213, the widest separation gravitational lens system discovered by the Cosmic Lens All-Sky Survey. Radio imaging using the VLA at 8.46 GHz and MERLIN at 5 GHz shows two compact components separated by 4.56 arcsec with a faint third component in between which we believe is emission from a lensing galaxy. 5-GHz VLBA observations reveal milliarcsecond-scale structure in the two lensed images that is consistent with gravitational lensing. Optical emission from the two lensed images and two lensing galaxies within the Einstein radius is detected in Hubble Space Telescope imaging. Furthermore, an optical gravitational arc, associated with the strongest lensed component, has been detected. Surrounding the system is a number of faint galaxies which may help explain the wide image separation. A plausible mass distribution model for CLASS B2108+213 is also presented.     

J2EE在电力系统工作票信息化管理中的应用--从C/S模式到B/S多层模式的转换

介绍了传统C／S模式在电力工作票管理信息系统中的应用及其问题，同时介绍J2EE多层分布式体系结构在工作票管理系统中应用的可行性。通过对传统C／S电力系统工作票管理系统的分析，提出将J2EE应用于工作票管理系统的思想并进行实践。     

Interaction between nulls and emission in the pulsar B0834+06

We present a detailed study of the single pulses of the bright radio pulsar B0834+06, and offer evidence that the dominant periodic modulation in this pulsar's emission governs the occurrence of nulls. The nulls of B0834+06 constitute approximately 9 per cent of the total pulses and we demonstrate that they do not occur at random in the pulse sequence. On the contrary, they are found to occur preferentially close to the minimum of the pulsar's emission cycle, whose period jitters around a central value of P ₃≈ 2.17 rotation periods. It is likely that the intrinsic duration of the nulls averages about 0.2 times the pulsar rotation period. Surprisingly, the clearly distinct population of nulls and partial nulls of B0834+06 exhibit a two-peak profile slightly broader than that of the normal emission. This is in contrast to the profile of extremely weak normal pulses, which is narrower than the overall profile. A flow/counterflow model for the pulsar's two components can reproduce the essential observed features of the emission in its dominant mode, with nulls occurring at the point where the minima of the two systems are aligned. This suggests that the observed nulling rate is determined by the chance positioning of our sightline with respect to the system. If the flow is interpreted as part of a circulating carousel, a fit yields a best estimate of 14 'sparks'.     

西藏扎布耶盐湖超大型B、Li矿床成矿物质来源研究

扎布耶盐湖位于西藏高原腹地,是一个现代盐湖矿床。对扎布耶地区地球化学背景的研究表明:变质岩及蚀变岩石中硼锂含量很高以及电气石脉的出现,暗示着扎布耶地区深部曾产生含硼锂高的热流体;沉积岩中除晚石炭世砂岩含硼锂稍高外,其他岩石均低于同类岩石的平均含量;火山岩中除早白垩世基性岩的硼锂含量高于基性岩平均含量外,其他均很低;该区大量发育的第四纪钙华含硼锂非常高,表明早期的热水系统曾提供过大量的成矿物质;河流及泉水中的硼锂含量是世界河水平均含量的数倍至数百倍,表明地表和近地表条件下的水-岩相互作用的产物也是成矿物质来源之一。     

Analysis of UVB values in the centre of the Iberian Peninsula

Records of UV data started in Madrid at the beginning of the 90's decade. After some quality control on the data a seven year period from 1996 to 2002 was selected to perform an analysis of daily and seasonal variability of solar ultraviolet B (UVB) values at the centre of the Iberian Peninsula. Instruments used are a Brewer MKIV spectrophotometer and a YES UVB-1 broadband pyranometer. Both instruments provided integrated daily values according with the Diffey spectrum although they have different measurement procedures. Data statistics from each instrument for the same period and statistical relationships between daily values from both instruments are shown. As broadband YES provided a record with fewer time gaps, analysis of UVI extreme values is performed using that instrument. The relationship between UVB values with ozone, cloudiness and visible radiation has been described in several papers for different places in the world. In this paper, those relationships are shown for Madrid. A discussion about specific problems found when trying to isolate every effective factor is also included. Some of those relationships could be helpful to retrieve UVB values from other ancillary data as visible radiation and cloudiness. Finally, a detailed study for 10 days in June 1997 when the maximum record of daily values from the present time series was obtained, highlight the close correlation between total ozone content and the daily variability of UVB for similar amounts of incoming radiation.     

The 1997 periastron passage of the binary pulsar PSR B1259−63

We report here on multifrequency radio observations of the pulsed emission from PSR B1259−63 around the time of the closest approach (periastron) to its B2e companion star. There was a general increase in the dispersion measure (DM) and scatter-broadening of the pulsar, and a decrease in the flux density towards periastron although fluctuation in these parameters were seen on time-scales as short as minutes. The pulsed emission disappeared 16 d prior to periastron and remained undetectable until 16 d after periastron.
The observations are used to determine the parameters of the wind from the Be star. We show that a simple model, in which the wind density varies with radius as r ⁻², provides a good fit to the data. The wind is highly turbulent with an outer scale of ≤10¹⁰ cm and an inner scale perhaps as small as 10⁴ cm, a mean density of ∼10⁶ cm⁻³ and a velocity of ∼2000 km s⁻¹ at a distance of ∼50 stellar radii. We find a correlation between DM variations and the pulse scattering times, suggesting that the same electrons are responsible for both effects.