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151.
张雷 《西安航空技术高等专科学校学报》2014,(6):22-25
在全球化的文化背景下,公共传媒对传统的思想道德、文化底线产生着强大的冲击,而青年学生又是公共传媒的主要受众群体和组成部分。基于当前形势,针对新兴媒体对大学生思想政治教育所产生的影响开展了相应的调查和研究,提出了新形势下高校大学生思想政治教育的思路。调查结果显示:新兴媒体已经对大学生的学习、生活产生了较大的影响,高校应该开辟多种渠道以适应新兴媒体对高等院校思想政治教育所提出的新要求。 相似文献
152.
153.
Caroline Andrade Enner Alcântara Nariane Bernardo Milton Kampel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(7):2175-2188
Monitoring chlorophyll-a (Chl-a) concentrations in inland waters is crucial for water quality management, since Chl-a is a proxy for phytoplankton biomass and, thus, for ecological health of a water environment. Chl-a concentration can be retrieved through the inherent optical properties (IOPs) of a water system, which, in turn, can be remotely sensed obtained. Quasi-analytical algorithm (QAA), originally developed for ocean waters, can also retrieve IOPs for inland waters after re-parameterizations. This study is aimed at assessing the performance of sixteen schemes composed by QAA original and re-parameterized versions followed by models that use absorption coefficients as inputs for estimating Chl-a concentration in Ibitinga reservoir, located at Tietê River cascading system, São Paulo State, Brazil. It was verified that only QAAV5 based schemes were able to obtain reasonable estimates for image data and that by four models tested presented similar and acceptable results for QAAV5 outputs. The best model were applied to a Ocean and Land Colour Instrument (OLCI) image. Light absorption in the reservoir showed to be dominated by colored dissolved organic matter (CDOM), and wide spatial and temporal variability of optical and water quality properties was observed. 相似文献
154.
N.A. Zakaria S.H.M. Yusoff N.A.M. Rizal N.S.A. Hamid M.H. Hashim Z. Mohd Radzi M.H. Jusoh A. Yoshikawa T. Uozumi S. Abe 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(7):2199-2206
MAGDAS PEN was established on 19th September 2019 as one of the MAGDAS observatory arrays located at Universiti Sains Malaysia (USM) (5.15°, 100.50°). The main objective of the MAGDAS project is to monitor global electromagnetic and the ambient plasma density in the geospace environment. This installation has contributed to a better understanding of the Sun-Earth coupling system. This paper presents the installation process of one of the MAGDAS magnetometers named YU-8 T magnetic sensor and provides a preliminary analysis of geomagnetic HDZ components amplitude-time that was observed at PEN station. A one-month HDZ-geomagnetic field data was processed from 1st November to 30th November 2019. The daily variations with a consistent pattern in delta H geomagnetic field components are observed throughout the day with eastward electric field effects that are observed during solar peak hours. The delta H-component gradually increases around 0700LT and reaches the maximum reading at 1300LT with a range of value ~ 40-70nT. The value slowly decreases that started from 1400LT until the night time. The reading during the night time shows a constant variation with magnitude varies in between ?10nT to + 10nT. The average H-component value of the night time is used as the baseline for the observation system. Overall, the observed trends portray a good sign of solar quiet field and Sq with no solar-terrestrial disturbances. 相似文献
155.
V.V. Kalegaev N.A. Vlasova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Dynamical features of proton fluxes at high and middle latitudes were studied based on data measured by Sun-synchronous low-altitude (800 km height) polar-orbiting three NOAA series satellites: POES 15, 16, and 17 during the geomagnetic storm on January, 21–22, 2005. Data from three satellites that passed the Northern hemisphere along different MLTs allow reconstructing the longitudinal distribution of the proton fluxes. Measurements of protons with energies of 30–80 keV and 80–240 keV (the ring current energy range) by 0- and 90-detectors were used to evaluate and compare the longitudinal asymmetry of proton flux distribution measured in the regions equatorward and poleward of the isotropic boundary. It was found that during all the phases of the geomagnetic storm distribution of the maximum flux of precipitating protons (0-detector data) is sufficiently asymmetric. The maximal flux position along MLT is moving from pre-midnight sector in quiet time to post-midnight one before and during SSC and moving back during recovery phase. The longitudinal distribution of precipitation maxima demonstrates the local increase in afternoon sector (approximately at 13:30 MLT) and decrease in the dusk one during SSC. These features are evident consequence of the magnetosphere compression. To identify the origin of the particles, the locations of maximum fluxes have been projected to the magnetosphere. It was determined that during geomagnetic storm main and recovery phases maximum fluxes were measured at latitudes poleward of the isotropic boundary. To evaluate the trapped particle flux asymmetry, the particle fluences (90-detector data) were calculated along the satellite orbit from L = 2 to the isotropic boundary. The total fluences of trapped particles calculated along the satellite orbit show regular asymmetry between dusk and dawn during main and recovery phases. The maximal intensity of proton fluxes of both investigated populations located poleward and equatorward of the isotropic boundary is achieved during SSC. The total flux measured during crossing the anisotropic region can be considered as a proxy for ring current injection rate. 相似文献
156.
157.
尹婷婷 《西安航空技术高等专科学校学报》2013,(5):88-91,96
以2013年我院教师思想状况滚动调查问卷调查结果和座谈情况为依据,对在当前的社会环境、文化环境下,我院教师思想状况呈现出的现状和趋势进行了分析,对思想状况的产生原因进行了剖析,并提出了改进思想状况的相关建议。 相似文献
158.
为进一步分析、了解高职院校贫困学生的基本状况,寻求更有效的、更有针对性的贫困学生资助办法,以福建卫生职业技术学院为例,建立并完善贫困学生档案数据库,发放学生评价体系和资助体系调查问卷,综合了解、分析贫困学生的基本现状并提出相应对策。 相似文献
159.
分析CAPP系统在航修企业中的应用现状及存在的问题,总结航修企业工艺设计对CAPP系统提出的要求,论述开发CAPP系统的步骤和在CAPP系统开发中应注意的问题。 相似文献
160.
采用已经建立的环电流离子解析模型,结合Chamberlain地冕中性层模型,研究了2004年11月一次大磁暴期间的环电流区域中性原子(ENA)图像.结果表明,模拟的ENA图像与TC-2卫星搭载的中性原子成像仪(NUAUD)的观测图像在方位角或地方时分布、高度或纬度分布和能谱分布方面存在一定的差异.如果依据磁暴发展的不同阶段来选择环电流离子模型的方位角不对称因子和通量最大方向的方位角,增大地冕中性层在低高度区域的密度或者考虑氢(H)以外的其他中性成分,改进注入边界处的离子能谱分布函数,且考虑不同种类环电流离子的比例随磁暴发展可能发生的变化,该模型有望产生更符合观测的模拟ENA图像. 相似文献