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151.
从球坐标系出发,利用三角形余弦定理和大气折射理论,推导了不作任何近似的、包含地球曲率和大气折射影响的多普勒天气雷达波束水平距离D_m的计算公式,并与斜距投影D_r、地表平面近似的计算公式(不考虑地球曲率和大气折射,记为D_d)和地表球面近似的计算公式(不考虑大气折射,记为D_s)进行了对比分析。结果发现,在标准大气状态下,D_m与D_r在高仰角相差2.5 km以上(D_r大),最高距离差达3.5 km(19.5°仰角最大斜距处);与D_d在低仰角相差0.5 km以上(D_d大),与D_r相差在0.5 km以下(Dm大)。并利用2011—2015年南昌站的探空资料,分析了南昌地区各个季节大气折射的变化情况及其与标准大气的区别。结果显示,夏季南昌上空电磁波的传播受大气折射的影响最大,冬季电磁波受大气折射的影响最小。最后,给出了南昌地区各个季节地球曲率K及等效地球半径Rm与标准大气的订正关系。 相似文献
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153.
采用城市化的多项要素指标,系统考察了太原1980-2009年期间城市化的发展对其城市热岛效应的影响关系,发现城市化的发展是导致城市热岛效应形成和加剧的主要原因.认为:①近30年,太原市郊区的增温率为0.51℃/10a,市区的增温率为0.90℃/10a,热岛强度的增温率为0.39℃/10a,热岛效应不断增强;②各类城市发展指数与城市热岛效应都有很好的相关关系;③太原城郊温差和总人口对数呈线性相关关系,其长期变化相关系数为0.81;④太原城郊温差和城市房屋建筑面积对数呈线性关系,其长期变化相关系数为0.85. 相似文献
154.
Fen-Fei Wang Jian-Jun Liu Chun-Lai Li Xin Ren Ling-Li Mu Wei Yan Wen-Rui Wang Jing-Tao Xiao Xu Tan Xiao-Xia Zhang Xiao-Duan Zou Xing-Ye Gao 《中国天文和天体物理学报》2014,(12)
The establishment of a lunar control network is one of the core tasks in selenodesy, in which defining an absolute control point on the Moon is the most important step. However, up to now, the number of absolute control points has been very sparse. These absolute control points have mainly been lunar laser ranging retroreflectors, whose geographical location can be observed by observations on Earth and also identified in high resolution lunar satellite images. The Chang'e-3(CE-3) probe successfully landed on the Moon, and its geographical location has been monitored by an observing station on Earth. Since its positional accuracy is expected to reach the meter level, the CE-3 landing site can become a new high precision absolute control point. We use a sequence of images taken from the landing camera, as well as satellite images taken by CE-1 and CE-2, to identify the location of the CE-3 lander. With its geographical location known, the CE-3 landing site can be established as a new absolute control point, which will effectively expand the current area of the lunar absolute control network by 22%, and can greatly facilitate future research in the field of lunar surveying and mapping, as well as selenodesy. 相似文献
155.
Jian-Qing Feng Jian-Jun Liu Fei He Wei Yan Xin Ren Xu Tan Ling-Ping He Bo Chen Wei Zuo Wei-Bin Wen Yan Su Yong-Liao Zou Chun-Lai Li 《中国天文和天体物理学报》2014,(12)
The Extreme Ultraviolet Camera(EUVC) onboard the Chang'e-3(CE-3)lander is used to observe the structure and dynamics of Earth's plasmasphere from the Moon. By detecting the resonance line emission of helium ions(He+) at 30.4 nm, the EUVC images the entire plasmasphere with a time resolution of 10 min and a spatial resolution of about 0.1 Earth radius(RE) in a single frame. We first present details about the data processing from EUVC and the data acquisition in the commissioning phase, and then report some initial results, which reflect the basic features of the plasmasphere well. The photon count and emission intensity of EUVC are consistent with previous observations and models, which indicate that the EUVC works normally and can provide high quality data for future studies. 相似文献
156.
Similar to the case of pulsars the magnetic axis and the spin axis of gamma-ray burst sources may not lie on the same line. This may cause the formation of a ring-like jet due to collimation of the processing magnetic axis. We analyze the tail emission from such a jet, and find that it has a shallow decay phase with a temporal index of -1/2 if the Lorentz factor of the ejecta is not very high, which is consistent with the shallow decay phase of some early X-ray afterglow detected by Swift. The ring-like jet has a tail cusp with sharp rising and very sharp decay. This effect can provide an explanation for the re-brightening and sharp decay of the X-ray afterglow of GRB 050709. 相似文献
157.
1 IntroductionTheArcticarea ,asthebackgroundofglobalclimateandenvironment,drawspeo ple’sattentionwithitsimpactonglobalchange (IPCC 1 990 ) .Greatamountofenergyandmassareexchangedbetweentheseaandairwithspecialinterface,air ice seasurface ,inthisarea .Thereforeiti… 相似文献
158.
Chen Cao Hong Wu Jian-Ling Wang Cai-Na Hao Zu-Gan Deng Xiao-Yang Xia Zhen-Long Zou National Astronomical Observatories Chinese Academy of Sciences Beijing Graduate School of Chinese Academy of Sciences Beijing College of Physical Sciences Graduate School of Chinese Academy of Sciences Beijing Department of Physics Tianjin Normal University Tianjin 《中国天文和天体物理学报》2006,6(2):197-209
We selected a sample of luminous infrared galaxies by cross-identification of the Faint Source Catalogue (FSC) and Point Source Catalogue (PSC) of the IRAS Survey with the Second Data Release of the SDSS. The size of our sample is 1267 for FSC and 427 for PSC by using the 2σ significance level cross-section. The "likelihood ratio" method is used to estimate the individual's reliability and for defining two more reliable subsamples (908 for FSC and 356 for PSC). A catalog of infrared, optical and radio data is compiled and will be used in further work. Some statistical results show that luminous infrared galaxies are quite different from ultra-luminous infrared galaxies. The AGN fractions of galaxies at different infrared luminosities and the radio-infrared correlations are consistent with the previous studies. 相似文献
159.
1 IntroductionArcticclimateandenvironmentareveryimportantintheglobalchangesystems(WMO/UNEP 1 990 ;WMO 1 991 ) .Observationsandmodelingresultsindicatethattheglobalwarmingwillbeenhancedinthepolarregions ,especiallyintheNorthHemi sphere ,withapredictedwarmingofabout… 相似文献
160.