共查询到18条相似文献,搜索用时 31 毫秒
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《地球物理学报》2005,(1)
(2 0 0 4年 9月 1 9~ 2 5日 ,武夷山 )第五次空间天气学研讨会暨“中国科学院空间天气学研讨会” ,也是第一次国际日地系统气候和天气计划空间天气主题研讨会 (TheFirstChineseSpaceWeather/CAWSESSymposium) ,由国家自然科学基金委员会地球科学部和中国科学院主办 ,中国科学院空间科学与应用研究中心具体组织、承办 .出席会议的人数为 16 1人 ,其中院士 7人 .会议由中国科学院空间科学与应用研究中心魏奉思研究员和国家自然科学基金委员会地球科学部地球物理和空间物理学科主任于晟博士共同主持 ,各单元的学术报告由刘振兴院士和中国… 相似文献
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第二次全国空间天气学研讨会于1998年8月7日至13日在黄山举行,这次会议是由国家自然科学基金委地球科学部、信息产业部22所和中国科学院空间科学与应用研究中心"日球物理数值研究开放实验室"联合主办,来自总参气象局、总参通信部、航天部、信息产业部、高校、地震局、海洋局和中国科学院等部门所属20余个单位80余位代表参加了会议.国家科技部基础司邵立勤副司长到会作重要讲话,他指出,空间天气学是一门跨世纪的新学科,从现在起应予重视,好好策划.空间天气是指太阳表面、太阳风、磁层、电离层和热层中影响空间、地面技术系统的运行和… 相似文献
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2004年全球灾害地震的灾情综述 总被引:1,自引:0,他引:1
根据美国地质调查局国家信息中心的互联网数据,2004年1月1日~12月31日,全球共发生M≥6地震156次。其中M≥7地震16次,M≥8的地震2次。M≥9的地震1次。M≥6的地震与最近10年(1990~2000年)期间的年平均数153次相近。比近100年来(1900~1999年)的年平均数126次高。 相似文献
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日冕物质抛射—空间天气的扰动源 总被引:5,自引:0,他引:5
日冕物质抛射是引起空间天气扰动的重要起因_本文对日冕物质抛射的一般参量和形态、它与其它太阳活动现象的关系、它在行星际空间的表现以及它导致的地球空间环境扰动的研究进展作了介绍和讨论 相似文献
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为了消除地震资料空间采样不够造成的空间假频现象,在claerbout空间2-D预测误差滤波器的启示下,本文提出了空间域位置相关法道内插值,在地面实际资料处理中都取得了良好的效果。 相似文献
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Summary of Global Earthquake Disasters in 2018 总被引:1,自引:0,他引:1
According to global seismic hazards data in 2018, the paper summarizes major hazards data of the global earthquakes, describes the major seismic hazards, and analyzes the characteristics of disasters losses of hazard earthquakes in this year. Focusing on the disaster and the cause of the September 28, 2018, Indonesia earthquake, and listing the major earthquakes triggered the tsunami disasters in history. Finally, giving suggestions and measures to deal with the earthquake disasters effectively. 相似文献
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M. Yu. Ortikov V. A. Shemelov I. V. Shishigin B. V. Troitsky 《Journal of Atmospheric and Solar》2003,65(16-18):1425-1430
The method for estimating an ionospheric index of solar-activity (IISA) based on the processing of spacecraft radio signals is suggested. The IISA values have been obtained by comparison between the measured and calculated variations of radio-signal characteristics. To calculate the variations of radio-signal characteristics, the straight rays approximation and the solar-activity index (Wolf numbers W and/or values of F10.7 solar flux) as a control parameter of the ionospheric model have been used. The suggested method was tested using spacecraft radio signals from the radio-navigation system “CIKADA”. The reduced differences of phases (ΔΦ) for frequencies 150 and 400 MHz were measured and the same characteristics were calculated by integration along the ray of radio-wave propagation between the receiver and the satellite. The IRI-95 has been used as a background ionospheric model. The satellite co-ordinates were determined using the orbit parameters recorded in the navigation messages. Minimization of the difference measured and calculated ΔΦ using arbitrary time steps, or during whole time intervals of observation, gives the IISA corresponding the satellite pass. Daily IISA values were obtained by averaging over all communication contacts during a day (20–30 passes). Testing this approach based on the measurements during March/April 1997, 1998, shows that on magnetically quiet days differences between IISA and the primary solar activity indices are about 5%. 相似文献
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Geomagnetically induced currents (GIC) in technological systems, like electric power transmission grids, at the Earth's surface are caused by space weather processes, whose origin is in the Sun. In power systems, transformers may be saturated due to GIC leading to different problems extending from an increase of harmonics to a blackout of the system and damage of transformers. To design reasonable measures against impending problems, GIC magnitudes in the network should be estimated in different circumstances. This paper tackles basic features of GIC flow in a fictitious five-transformer/four-line power system, which is simple enough to make the equations easily manageable but complex enough to yield real and usable information. It is shown that the direction of the geoelectric field affects GIC at different sites but the dependence is not straightforward since GIC produced in one part of the system flows to others. Generally, transmission lines experience much larger GIC than transformers. Series capacitors in transmission lines prevent the flow of dc-like GIC but, without a careful analysis, their installation may result in larger GIC at some transformers of the system thus increasing the risk of problems. 相似文献