在97.8GHz处测量地球大气的不透明度

用研制的全自动辐射计在97．8GHz上测量南京市内大气的不透明度以及这种不透明度随时间的变化．辐射计记录大气在不同天顶高度的辐射温度,由此测出天顶方向的大气不透明度。在56小时的测量时间内,取得了1400多组数据,拟合得到了在观测时段内天顶方向的大气不透明度在0．2至0．7之间,典型值为0．4,表明测试地点的大气条件允许进行3mm波段的射电天文观测．由于在工作频段内大气不透明度的主要来源是对流层水汽的吸收,测量的不透明度可用来直接反映大气内水汽的含量,并实时校准大气吸收．     

流动注射—二苯硫脲纤维素在线富集——火焰原子吸收法测定地质样品？…

本研究采用自行合成的二苯硫脲纤维素作为在线富集介质,流动注射与原子吸收法联用快速测定地质样品中痕量金,在本法选定条件下,测定速度为３０样／ｈ,测定灵敏度为０．３１μｇ／ｍｌ（１％吸收）,ＲＳＤ为２．５９％。     

光石汉含铀花岗伟晶岩成因探讨

本文研究了光石沟含铀花岗伟晶岩的构造环境、成岩物质来源和形成方式,并运用微量元素定量模型模拟了其形成过程。研究表明,花岗伟晶岩是在大陆火山弧环境,由８９．７％的秦岭群和１０．３％的上地幔物质,经３５％左右部分熔融形成的重熔岩浆结晶分异而成。     

水稻田间小气候特点与生产潜力关系研究

通过稻田小气候与水稻生长发育的平行观测,探索水稻优质高产的田间小气候特征,分析表明,稻田小气候效应,符合局部气候原理和田间小气候基本规律。在采用岗优２２组合,密用２．２５万窝／ｈｍ＾２的稻田里,生长发育的关键期－抽穗开花期,能形成更为合理的田间小气候,水温,地温和气温配合较优,光照较好,有利于ＣＯ２的输送,增强了光合２作用和有机质的积累,因而对光能的利用率较高,能达到１０４１０ｋｇ／ｈｍ＾２的产量     

火焰原子吸收法测定大理岩中的锰

本文研究了大理岩中锰的火焰原子吸收测定方法。大量钙的存在干扰锰的测定，试验确定采用饱和消除法，效果良好。本法的精密度（RSD）为5．51％，试样加标回收率为99．4％。[第一段]     

Tests and applications of an approach to absorbing reflected waves towards incident boundary

If the upstream boundary conditions are prescribed based on the incident wave only, the time-dependent numerical models cannot effectively simulate the wave field when the physical or spurious reflected waves become significant. This paper describes carefully an approach to specifying the incident wave boundary conditions combined with a set sponge layer to absorb the reflected waves towards the incident boundary. Incorporated into a time-dependent numerical model, whose governing equations are the Boussinesq-type ones, the effectiveness of the approach is studied in detail. The general boundary conditions, describing the down-wave boundary conditions are also generalized to the case of random waves. The numerical model is in detail examined. The test cases include both the normal one-dimensional incident regular or random waves and the two-dimensional oblique incident regular waves. The calculated results show that the present approach is effective on damping the reflected waves towards the incident wave boundary.     

Variable Star Status of Two Stars： V204 and I-I-39 in M3

The star 1-1-42 （=vZ1390）, a cluster member in M3, located near the red edge of the instability strip of the horizontal branch, was discovered by Roberts and Sandage as a low amplitude variable, it was designated as V204 in the ＂second catalogue of variable stars in globular clusters＂, but its coordinates given in all versions of this catalogue are wrong since 1955. We argue that V204 is indeed a low amplitude HB variable star, located near to the red edge of the instability strip, with a period of 0.74785d and an amplitude of about 0.04 mag in V. We also find that the red cluster member star 1-1-39 is a low amplitude variable with a period of 1.16^d and amplitude of about 0.03 mag in V which might be pulsating at the second overtone.     

预啁啾和脉冲沿锐度对光脉冲线性传输的影响

从忽略光纤非线性效应的光脉冲非线性薛定谔方程出发,在光纤正色散区,利用傅立叶变换和反傅立叶变换模拟了不同初始啁啾的二阶与四阶超高斯光脉冲波形随距离的三维演化.分析讨论了脉冲沿锐度以及脉冲预啁啾对脉冲波形演化的综合影响.结果表明:不论脉冲有无预啁啾,光脉冲波形最终都将随着传输距离的增大而展宽.但是负预啁啾将使脉冲波形在脉冲传输的初始阶段发生严重的畸变,即脉冲会分裂成尖峰结构,并且尖峰的数目和能量分布随距离而变.而当预啁啾为正或零时,脉冲前期的畸变很弱.随着脉冲沿锐度的增大,脉冲畸变会加强.此外,在脉冲的前后边缘会出现矮小的峰.整个脉冲波形都是中心对称的.