基于两种数据传输途径的国家级地面自动站逐小时数据差异分析     

张志富  任芝花  邹凤玲 《气象与环境学报》2014,30(1):64-68

对2006-2009年两种途径（A文件和Z文件）上传的2400多国家级自动站观测的小时常规六要素资料进行了对比分析。结果表明：两种途径得到的小时数据中,2 min风和10 min风的不一致率较高,主要由两种文件对于风速为零时风向的规定不同造成,其他要素的不一致率相对较低;在不一致数据中,各要素在仪器误差允许范围内的比率分别为气温23.27 %、气压5.4 %、相对湿度23.19 %、降水65.42 %、2 min风12.93 %、10 min风14.16 %。  相似文献   

三疣梭子蟹HMGR基因的克隆及其在蜕皮中的表达分析   总被引：2，自引：1，他引：1  

邱锡尔  朱冬发  崔晓雨  汤洁  谢熙 《海洋与湖沼》2014,45(6):1192-1201

为了研究3-羟基-3-甲基戊二酰辅酶A还原酶(3-hydroxy-3-methyl glutaryl coenzyme A reductase,HMGR)在甲壳动物蜕皮调控中的作用,采用RT-PCR和c DNA末端快速扩增技术(RACE),克隆得到三疣梭子蟹(Portunus trituberculatus)HMGR基因的c DNA序列(Gen Bank登录号:KF280756)。该序列全长2575bp,包括一个53bp的5′端非编码区,一个686bp的3′端非编码区和一个长度为1836bp的开放阅读框,编码611个氨基酸。该氨基酸序列与已公布的美洲海鳌虾HMGR氨基酸序列相比一致性达65%,具有Ⅰ型HMGR保守催化区域、两个HMG-Co A结合基序和两个NADP(H)结合基序。采用实时荧光定量PCR(q RT-PCR)技术,分析三疣梭子蟹HMGR基因的组织差异表达及在蜕皮周期中的表达水平变化,结果表明HMGR基因在三疣梭子蟹大颚器(MO)中的表达量最高,在其它组织中表达量均极低;在三疣梭子蟹蜕皮周期中,大颚器中HMGR基因的表达量自A期至D0亚期升至最高,然后下降,至D4亚期最低。验证了大颚器是三疣梭子蟹合成甲基法尼酯的唯一器官,表明HMGR在三疣梭子蟹蜕皮调控中起着重要作用。  相似文献   

NNR������ITRF��ȫ�����˶�ģ��   总被引：1，自引：0，他引：1  

张西光  吕志平  赵冬青 《大地测量与地球动力学》2007,27(3):39-43

????????ITRF2000???????????????????????????ITRF2000??1 mm/a????????????NNR??NUVEL1A?????????????NNR????;??????????????????????????????????ж?ITRF??????????NNR??????  相似文献   

甘草和连翘对牙鲆CYP3A 活性影响的研究     

韩现芹  李健  李吉涛 《海洋科学》2010,34(12):19-25

研究甘草(Glycyrrhiza uralensis)和连翘(Forsythia suspensa)对牙鲆(Paralichthys olivaceus)肝细胞色素P4503A(CYP3A)活性的影响。将牙鲆随机分为3组,即对照组、甘草组和连翘组,对照组每日口灌0.9%的生理盐水,试验组每日1次口灌甘草30 mg/kg和连翘100 mg/kg,连续口灌6 d,第7天时,采用直接测定法和间接测定法(探针药物)进行CYP3A酶活性的测定。结果显示:在肝微粒体水平上,甘草和连翘均可明显提高红霉素-N-脱甲基酶活性,分别提高了1.79倍、4.87倍。与对照组相比,甘草组和连翘组氨苯砜的半衰期分别降低了4.51%(P0.05)和36.8%(P0.01);药时曲线下面积分别减小了8.28%(P0.05)和32.3%(P0.01);总清除率分别增加了5.63%(P0.05)和99.3%(P0.01)。说明连翘对牙鲆CYP3A的活性具有极显著诱导作用,甘草诱导作用不显著。提示其他药物与连翘合用时,其有效性和安全性可能会受到影响。  相似文献   

油企业抗震防灾规划信息管理系统的设计          下载免费PDF全文

《地震地质》1999,21(3):285

基于石油企业抗震防灾工作对网络与数据库的信息管理系统的需求，对数据库产品进行了简要分析，并根据石油企业抗震防灾规划的需求和信息管理的一般模式，提出了石油企业抗震防灾规划信息计算机管理系统的设想。认为，以 Ｍｉｃｒｏｓｏｆｔ Ａｃｃｅｓｓ 数据库软件为基础，利用 Ｖ Ｂ或 Ｖ Ｃ等可视化前端应用开发工具，是目前比较好的方案，它将使石油企业抗震防灾规划工作在办公自动化方面迈向新的台阶  相似文献   

Observations of pulsating Ap stars in South Africa     

Peter Martinez  D. W. Kurtz 《Astrophysics and Space Science》1995,230(1-2):29-39

The rapidly oscillating Ap (roAp) stars currently represent the only main sequence stars other than the Sun which exhibit non-radial acoustic pulsations of high overtone. This makes them excellent subjects for asteroseismology, an approach which promises to yield accurate knowledge of the interior structures of stars. Of the 27 known roAp stars, 24 were discovered in Sutherland despite extensive searches conducted elsewhere. This paper reviews the discovery of the roAp phenomenon and describes the factors that contribute to the high discovery rate for these stars at Sutherland. Two long-term observational projects in progress at Sutherland are discussed,viz. the Cape roAp Star Survey and long-term monitoring of frequency variations in roAp stars.  相似文献   

Photopolarimetry of 3C 66A in 2003     

Yu. S. Efimov  N. V. Primak 《Astrophysics》2006,49(1):36-53

The BL Lac-type object 3C 66A was observed at the Crimean Astrophysical Observatory during the international project OJ-94. Observations were made over 10 nights from February through December 2003 at the Cassegrain focus of the 125-cm AZT-11 telescope with a photopolarimeter capable of simultaneous measurements in the UBVRI bands. In the course of our measurements the brightness of the object increased by more than 1 magnitude in all these bands. Its color indices varied and the degree of polarization decreased from ∼16% in February to ∼3% at the end of our observations. In December 2003 a rapid change in the position angle from 15° to 40° was noticed. The spectral energy distribution F_n is well described by a power law with a spectral index a (F_ν ∝ ν ^−α . The increase in brightness was accompanied by a reduction in the spectral index. The most probable mechanism for the observed changes in the brightness, degree of polarization, and spectral index may be a decrease in the magnetic field strength or a change in its configuration owing to a increase in the chaotic component of the field. __________ Translated from Astrofizika, Vol. 49, No. 1, pp. 41–59 (February 2006).  相似文献   

Merger Dynamics of the Pair of Galaxy Clusters——A399 and A401     

Qi-Rong Yuan  Peng-Fei Yan  Yan-Bin Yang  Xu Zhou Department of Physics  Nanjing Normal University  Nanjing yuanqirong@njnu. edu. cn National Astronomical Observatories  Chinese Academy of Sciences  Beijing Department of Mathematics  Physics  Qingdao University of Science  Technology  Qingdao 《中国天文和天体物理学报》2005,5(2):126-136

Convincing evidence for a past interaction between the two rich clusters A399 and A401 was recently found in the X-ray imaging observations. We examine the structure and dynamics of this pair of galaxy clusters. A mixture-modeling algorithm was applied to obtain a robust partition into two clusters, which allowed us to discuss the virial mass and velocity distribution of each cluster. Assuming that these two clusters follow a linear orbit and they have once experienced a close encounter, we model the binary cluster as a two-body system. As a result, four gravitationally bound solutions are obtained. The recent X-ray observations seem to favor a scenario in which the two clusters with a true separation of 5.4h-1 Mpc are currently expanding at 583 km s-1 along a direction with a projection angle of 67.5°, and they will reach a maximum extent of 5.65 h-1 Mpc in about 1.0 h-1 Gyr.  相似文献   

SN 1998A: explosion of a blue supergiant     

A. Pastorello  E. Baron  D. Branch  L. Zampieri  M. Turatto  M. Ramina  S. Benetti  E. Cappellaro  M. Salvo  F. Patat  A. Piemonte  J. Sollerman  B. Leibundgut  G. Altavilla 《Monthly notices of the Royal Astronomical Society》2005,360(3):950-962

We present spectroscopic and photometric observations of the peculiar Type II supernova (SN) 1998A. The light curves and spectra closely resemble those of SN 1987A, suggesting that the SN 1998A progenitor exploded when it was a compact blue supergiant. However, the comparison with SN 1987A also highlights some important differences: SN 1998A is more luminous and the spectra show bluer continua and larger expansion velocities at all epochs. These observational properties indicate that the explosion of SN 1998A is more energetic than SN 1987A and more typical of Type II supernovae. Comparing the observational data with simulations, we deduce that the progenitor of SN 1998A was a massive star  (∼25 M_⊙)  with a small pre-supernova radius  (≲6 × 10¹² cm)  . The Ba  ii lines, unusually strong in SN 1987A and some faint II-P events, are almost normal in the case of SN 1998A, indicating that the temperature plays a key role in determining their strength.  相似文献   

数字滤波技术在射电天文测量中的应用     

项英  张秀忠 《天文学进展》2004,22(2):95-103

随着数字技术的发展，数字信号处理芯片的速度越来越快，这为高速数字滤波的实时实现提供了可能。简要阐述了数字滤波的原理，并对两种数字滤波的实现方法进行了分析；给出了数字滤波较模拟滤波的优势；介绍了数字滤波在射电天文测量中的各种应用。  相似文献