青海省沙漠现状及形成与发展趋势   总被引：10，自引：5，他引：5  

李成尊  陆锦华 《中国沙漠》1990,10(4):38-45

本文根据遥感调查的结果,论述了青海省沙漠的类型、面积及分布规律特征。并通过不同时期的遥感图象,研究了青海湖等地区近三十年沙漠化环境的动态变化规律,从自然和人为因素两方面分析探讨了沙漠形成及发展趋势。  相似文献   

1989年1月18日白光耀斑的研究     

姜云春 《云南天文台台刊》1996,(1):86-87

本文利用色球Ｈα单色光序列照相资料，Ｈα光谱扫描资料，黑子精细结构照相资料和日面纵向磁场观测资料，分析了１９８９年１月１８日ＷＬＦ所在活动区ＮＯＡＡ／ＵＳＡＦ：５３１２的磁场结构，黑子结构及该ＷＬＦ的演化特征，求出了视向速度场，并以理论计算的Ｈα谱线轮廓作为诊断工具，探讨了该ＷＬＦ可能的能量传输机制和动力学过程。  相似文献   

LAMOST/GALAXY计划:利用LAMOST研究银河系     

胡景耀 《天文研究与技术》2004,1(3):234-240

本文讨论了利用LAMOST作银河系研究的科学意义及可能性；并提出具体实施LAMOST/GAIAXY计划的初步方案。  相似文献   

Sequences in the Hardness Ratio-Peak Energy Plane of Gamma-Ray Bursts     

Xiao-Hong Cui  En-Wei Liang  Rui-Jing Lu National Astronomical Observatories/Yunnan Observatory  Chinese Academy of Sciences  Kunming  ciwei@.com Department of Physics  Guangxi University  Nanning Department of Astronomy  Nanjing University  Nanjing Graduate School of the Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2005,5(2):151-158

The narrowness of the distribution of the peak energy of the vFv spectrum of gamma-ray bursts (GRBs) and the unification of GRB populations are great puzzles yet to be solved. We investigate the two puzzles based on the global spectral behaviors of different GRB populations, the long GRBs, the short GRBs, and the X-ray flashes (XRFs), in the HR - Ep plane (HR the spectral hardness ratio) with BATSE and HETE-2 observations. It is found that the long GRBs and the XRFs observed by HETE-2 seem to follow the same sequence in the HR-Ep plane, with the XRFs at the low end of this sequence. We fit the sequence by a universal Band function, and find that this sequence is mainly defined by the low energy index α, and is insensitive to the high energy index,β. With fixed β=-5, a best fit is given by α=-1.00 with X^2min/dof=2.2. The long and short GRBs observed by BATSE follow significantly different sequences in the HR-Ep plane, with most of the short GRBs having a larger hardness ratio than the long GRBs at a given Ep. For the long GRBs a best-fit yields α=-0.30 and β=-2.05. For the short GRBs, a best fit gives α=-0.60 with x^2min=1.1 (withβfixed at-2.0 because it is numerically unstable). The α value for the short GRBs is significantly greater than that for the long GRBs. These results indicate that the global spectral behaviors of the long GRB sample and the XRF sample are similar, while that of the short GRBs is different. The short GRBs seem to be a unique subclass of GRBs, and they are not the higher energy extension of the long GRBs.  相似文献   

充分利用卫星遥感技术积极探索现代土地变更调查新途径     

马素兰张玉敏  魏也纳 《河南国土资源》2003,(5):14-18

近年来,随着京九、宁西、漯阜铁路及京珠、连霍高速公路、小浪底水库、南水北调等一批国家重点项目在河南省的开工建设,有利地促进了我省经济、社会的发展,同时也使得土地利用现状发生了很大变化。由于人力、物力、财力的限制,我省大部分县(市、区)土地利用现状资料陈旧、破损、残缺,加上传统的土地变更调查技术和方法相对滞后,使每年的土地变更调查结果难以保持图、数、实地三者一致,土地利用现状的现势性和可靠性,已越来越难以满足国土资源管理和经济建设快速发展的需要。为此,非常有必要利用当前的先进技术手段,对我省土地利用现状进行一…  相似文献   

内蒙额仁陶勒盖银矿床含银性的红外光谱评价     

张培萍  朱钟秀 《长春地质学院学报》1993,23(3):319-322

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Magnetic Field Strengths and Structures from Radio Observations of Solar Active Regions     

Chang－XiZhang  G.B.Gelfreikh 《中国天文和天体物理学报》2002,2(3):266-276

Radio observations of some active regions (ARs) obtained with the Nobeyama radioheliograph at λ=1.76cm are used for estimating the magnetic field strength in the upper chromosphere, based on thermal bremsstrahlung. The results are compared with the magnetic field strength in the photosphere from observations with the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station of Beijing Astronomical Observatory. The difference in the magnetic field strength between the two layers seems reasonable. The solar radio maps of active regions obtained with the Nobeyama radioheliograph, both in total intensity (I-map) and in circular polarizations (V-map), are compared with the optical magnetograms obtained with the SMFT. The comparison between the radio map in circular polarization and the longitudinal photospheric magnetogram of a plage region suggest that the radio map in circular polarization is a kind of magnetogram of the upper chromosphere. The comparison of the radio map in total intensity with the photospheric vector magnetogram of an AR shows that the radio map in total intensity gives indications of magnetic loops in the corona, thus we have a method of defining the coronal magnetic structure from the radio I-maps at λ=1.76 cm. Analysing the I-maps, we identified three components: (a) a compact bright source; (b) a narrow elongated structure connecting two main magnetic islands of opposite polarities (observed in both the optical and radio magnetograms); (c) a wide, diffuse, weak component that corresponds to a wide structure in the solar active region which shows in most cases an S or a reversed S contour, which is probably due to the differential rotation of the Sun. The last two components suggest coronal loops on different spatial scales above the neutral line of the longitudinal photospheric magnetic field.  相似文献   

湘中锰矿控岩控矿构造遥感地质分析     

刘绍濂 《地质与勘探》1996,32(2):33-39

应用遥感信息结合其他地学资料综合分析湘中锰矿构造型式及控岩控矿地质特征，提出东西向和北东向同期构造与台地边缘相带共同控制锰矿的新认识。  相似文献   

遥感技术在构造地质研究及成矿预测中的应用     

杨武年  朱章森 《物探化探计算技术》1994,16(3):265-266

遥感技术在构造地质研究及成矿预测中的应用杨武年，朱章森（成都理工学院）本文应用现代化遥感技术，根据遥感多波段图像信息量大、对地质构造形迹显示的宏观性、信息连续性以及对隐伏构造具“透视”作用的特点，并据遥感横张大节理和剪切节理与宏观褶皱及断裂具有成因联...  相似文献   

超新星SN1993J的光谱观测     

胡景耀  姜晓军 《紫金山天文台台刊》1994,13(1):64-64,T004

SN1993J was first discovered by a Spanish amateur astronomer F. Garcia in NGC3031 (M81) on March 28, 1993. It's the closest supernova in the northern hemisphere since 1937. Because of its many special properties, it drove attentions of astronomers when it was discovered.  相似文献