BVRI CCD-Photometry of Comparison Stars in the Neighborhoods of Galaxies with Active Nuclei. II

Results are presented from CCD BVRI-observations of 145 comparison stars in the neighborhoods of 14 Seyfert galaxies, 3 quasars, and 5 BL Lac objects with right ascensions of 12 to 24 hours. The magnitudes of the observed stars ranged from V=11 to V=17. The typical photometric error for stars brighter V=14 is 0^m.01. The B, V, Rc, and Ic magnitudes of most of these stars were not known previously. 14′ x 14′ finding charts are provided. These results can be used for differential photometry of the nuclei of active galaxies in the B, V, Rc, and Ic bands.__________Translated from Astrofizika, Vol. 48, No. 3, pp. 365–379 (August 2005).     

A study of aerosol particle sizes in the atmosphere of Athens, Greece, retrieved from solar spectral measurements

This work aims at determining the aerosol particle radii in the atmosphere of Athens. Such a work is carried out in Athens for the first time. For this purpose, solar spectral direct-beam irradiance measurements were used in the spectral range 310–575 nm. To estimate the particle radius from aerosol optical depth retrieval, a minimization technique was employed based on the golden-section search of the difference between experimental and theoretical values of the aerosol optical depth. The necessary Mie computations were performed based on the algorithm LVEC.In this study, the mean particle radius of a given distribution was calculated every 30 min during cloudless days in the period November 1996 to September 1997. The largest particles were observed in the summer and the smallest during winter. The result was verified by the increased values of the aerosol optical depth and the turbidity factors calculated in the summer. The differences in the diurnal variation from season to season are attributed to the prevailing wind regime, pollutant emission and sink rates in the atmosphere of Athens.     

准格尔煤田特厚煤层开采底板破坏特征综合测试研究

鄂尔多斯盆地准格尔煤田某矿石炭-二叠系6煤层为特厚煤层,平均可采厚度17.0 m,其底板受到灰岩水的威胁。针对这种情况,现场采用分布式光纤传感及跨孔电阻率CT原位综合测试技术,先后获得了采动过程中多个工作面底板破坏应变场及地电场响应特征数据。结合岩样加载变形破坏的判别阈值参数及探测实践,对采区内4个工作面底板测试数据进行综合分析,获得了区内底板岩层破坏空间特征及其规律认识。分析认为底板破坏在垂向上具有明显的分带性,采区工作面底板破坏深度在7.2~16.5 m,主要破坏层位在细砂岩以上层段,扰动影响最大深度在33 m左右,主要扰动层位在砂质泥岩以上层段;底板破坏在横向上具有超前性,超前距离在25~60 m范围;区内工作面底板破坏特征具有一定的相似性,动压影响下的底板损伤程度在空间上呈东北区域浅、西南区域深的分布规律。原位测试所获得的数据对区内6煤层水害防治及安全开采具有指导作用。     

电子密码锁设计

在PROTEUS模拟仿真软件上,以AT89C51单片机为核心器件,结合按键电路、LED数码管显示电路、报警指示电路设计了一款保密性好、编码量多、随机开锁成功率几乎为零的电子密码锁。利用单片机灵活的编程设计和丰富的I／O端口,及其控制的准确性通过软件程序来控制整个系统实现电子密码锁的基本功能。系统能实现密码的输入、清除、显示,密码正确开锁,密码错误报警,系统设定初始密码。同时也显示了PROTEUS软件在硬件设计和软件调试方面的高效性。     

视错觉在地图制图中应用的研究

本文介绍了地图制图中常见视错觉现象的规律和原理,并对此在地图制图应用中作了一些初步探讨。合理地利用视错觉规律,\     

北京地区大气气溶胶光学特性监测研究

该文依据气溶胶光学厚度测量原理,利用CE318太阳光度计,于2000年7月～2001年7月期间对北京地区大气气溶胶光学厚度进行观测试验,计算得到约50天的气溶胶光学厚度和Junge参数等大气光学特性数据,给出了北京地区气溶胶光学特性分布特征.计算统计得到北京城区晴空条件下的Junge参数为3 15、2001年3月份沙尘天气状况下急剧下降为2.28,而北京郊区顺义县的测量结果介于二者之间为2.65.分析表明,由试验获得的气溶胶光学特性数据对于分析和监测北京地区大气污染、改善北京地区空气质量具有一定的意义.     

光学后向散射浊度仪简介及应用研究

主要介绍了进口光学散射浊度仪的结构、测量原理、校准，并对其误差和影响因素进行了分析，揭示了含沙浓度与浊度的相关关系，并结合在长江口中的应用提出其应用前景。     

山东气溶胶光学厚度时空分布及其与地面大气污染物质量浓度的相关性分析

基于卫星的气溶胶光学厚度(aerosol optical thickness,AOT)是研究大气污染程度及时空变化的重要参考,由于大气污染物排放特征、地理和气候背景不同,不同区域AOT的时空分布及其与地面大气污染物质量浓度的相关性存在一定的差异.选取了2017年7月-2020年7月山东89个国家环境空气质量监测站数据、...     

全球人为硫酸盐和烟尘气溶胶资料及其光学厚度的分布特征

简单介绍了两种不同化学输送模式及其输出的硫酸盐和/或烟尘气溶胶资料,初步分析了它们之间的异同。同时,在广泛搜集整理已有资料的基础上,给出了硫酸盐和烟尘气溶胶在整个太阳光谱0.2～40 μm波段内共72个间隔上的复折射指数资料;计算并分析了其整层光学厚度的全球分布特征。结果表明,无论是地理分布还是数值大小均基本合理。结合上述资料及计算结果,初步建立了一个全球硫酸盐和烟尘气溶胶资料库,该库对化学输送模式、辐射强迫和气候效应的研究都有参考意义。     

BVRI CCD-photometry of comparison stars in the fields of galaxies with active nuclei. IV

We report observations of 24 stars in the fields of the three Seyfert galaxies MCG +08-23-067, Mrk 817, and Mrk 290. The observations were made with a CCD array photometer in the BVRcIc bands. The V magnitudes of the observed stars ranged from 13.5 and 17.2. For stars of approximate magnitude 15, the typical photometric errors are 0.010, 0.011, 0.008 and 0.011 magnitude in the BVRI bands, respectively. The BVRI magnitudes of all these stars were not known previously. In the field of the galaxy Mrk 290 a star has been found that probably has a periodic brightness variation with P=1.518 days and the mean value V=14.80 and which may belong to the class of “spotted” stars. 14′x14′ charts are supplied for identifying the stars. These results can be used for differential photometry of active galactic nuclei in the BVRI bands. __________ Translated from Astrofizika, Vol. 51, No. 1, pp. 41–50 (February 2008).