microwave burst 微波爆发(19) 微波大爆发(6)   微波爆发      These FS were superimposed on the microwave burst.      这些FS都是叠加在微波爆发上的. 短句来源      OBSERVATIONS OF MICROWAVE BURST ON 15 APRIL,1998      1998年4月15日微波爆发观测 短句来源      The Spike-like Structure in A Solare Microwave Burst on May 21,1990      1990年5月21日微波爆发中的类尖峰辐射结构 短句来源      FINE STRUCTURE OF SOLAR MICROWAVE BURST AT SHORT-CENTIMETER WAVEBAND      短厘米波段太阳微波爆发中的精细结构 短句来源      A SOLAR MICROWAVE BURST SPECTROMETER      太阳微波爆发动态频谱仪 短句来源 更多          微波大爆发      Study of a Great Microwave Burst on December 16,1988      1988年12月16日微波大爆发的研究 短句来源      The Intense Microwave Burst Associated with a White Light Flare on June 6,1991      1991年6月6日与白光耀斑共生的微波大爆发 短句来源      A Big Complex Microwave Burst——Solar Radio Burst on Oct. 14 in 1980      一次形态复杂的微波大爆发——1980年10月14日射电爆发 短句来源      2. On April 1, 1981 the great microwave burst consists of three major bursts. The times of flux peaks are 0135.1 UT, 0146:1 UT and 0153.6 UT, respectively.      (2)4月1日微波大爆发是由三个主爆发组成的,它们的峰值时刻分别为0135.1,0146.1,0153.6UT. 短句来源      In this paper, the spikes and fast fine structures (FFS) superimposed on the microwave burst with the type 47GB on May 16, 1991 were introduced briefly.      本文简述了1991年5月16日叠加在一个47GB微波大爆发上的快速精细结构(FFS)和spike群的偏振状态. 短句来源 更多          “microwave burst”译为未确定词的双语例句      The Number of Energetic Electrons Deduced From a Type C Microwave Burst      从一个微波C型爆推算到的高能电子数 短句来源      Filtergrams of 1B/M1-M4 Ha flare starting at 22h25m of November 11, 1980 are digitized, and isophote lines are drawn in order to compare with hard X-ray, soft X-ray and microwave burst images.      本文对1980年11月5日22点25分开始的1B/M1-M4的Hα耀斑进行了图象处理,绘制了等光度图; 与硬、软X射线象,微波象进行了比较. 短句来源      The Classification of Solar Microwave Burst      太阳微波爆分类 短句来源      A Comparison Between Hard X-ray, Soft X-ray, Microwave Burst Images and Ha Isopfaote Map of Flare on November 5, 1980      1980年11月5日耀斑的硬、软X射线及微波的象与Hα等光度象的比较 短句来源      A Method of Generating Microwave Burst Frequency Spread Signal      一种产生微波突发扩频信号的方法 短句来源 更多        查询“microwave burst”译词为用户自定义的双语例句     我想查看译文中含有：的双语例句 为了更好的帮助您理解掌握查询词或其译词在地道英语中的实际用法，我们为您准备了出自英文原文的大量英语例句，供您参考。   microwave burst One of the quasi-periodically appearing patches is associated with the microwave burst emission, the same (or a later, lower frequency one) immediately preceeds the meter wave type II burst lanes. 例句来源       Microwave burst of November 17, 1991: Evidence of fragmented particle injection into a coronal loop 例句来源       Possible role of p-mode photospheric oscillations in modulation of microwave burst emission is discussed. 例句来源       The fact that the noise-storm decreases develop with delays of several tens of minutes relative to the associated microwave burst peak, when the corresponding CME front is located at heights of several R⊙, however, is not explained. 例句来源       The magnetic field strength is estimated on the basis of such a model in the microwave burst sources at ～ 100-200?G. 例句来源       更多                    The history of solar microwave busrt classification at home and abroad and the physical meanings of the classification are generalized, and the classification notes of 49 types used at present in S. G. D are listed in detail in this article. The microwave burst classification of Purple Mountains Observatory made in 1980 is systematically compared with that of Beijing Observatory, the reason of the discrepancy between them is found out and a proposal for the future classification work is of...             本文主要概述国内外太阳微波爆分类历史及分类的物理意义,并详细列出国际上太阳地球物理资料(SGD)目前使用的49分类的注释。还系统地比较了80年紫台、北台对微波爆分类工作,找到了分歧原因,提出今后分类工作的建议。 文摘来源          A flare of Importance 3B occurred at 0542-0613-0734 UT on 1980 Oct. 14 in a sunspot region (M. W. No 21811, AR2725) at S10/Wl5. During the flare, the spray, it's disturbance along an arc trajectory and the associated radio burst at the 3.2-cm and 10.6-cm wavelengths were observed at Beijing Observatory. The observations of Yunnan Observatory at the 8.2-cm wavelength, Tokyo Observatory at the 2-cm wavelength and Toyokawa at the 15-cm and 30-cm wavelengths, and the spectral data in SGD are used to analy...             1980年10月14日0542—0613—0734UT.,在位于日面S10W15的黑子区(M.W No.21811、AR2725)发生了一个3B级大耀斑。北京天文台的色球望远镜取得了比较完整的Hα观测资料,观测发现在耀斑爆发过程中存在喷焰(Spray)现象及扰动沿弧形轨迹运动的现象。北京天文台的3.2厘米(9395MHz),10.6厘米(2840MHz)总强度射电望远镜取得了完整的总辐射流量密度的时变曲线,参考云南天文台的8.2厘米及日本东京天文台2厘米,Tykw的15厘米,30厘米及S.G.D上的频谱资料对这一形态复杂的微波爆发作一初步的形态分析,与Hα资料作了比较,利用文献中的硬x线资料与射电资料作了初步的对比。 文摘来源          A .3B flare which occurred in a spotless region on Oct. 15, 1980 is rrio-phologically analysed in some detail. The main results of the analysis are as follows: 1) The flare had no flash phase and the maximum intensity of the flare was about 2.4 times as much as that of the undisturbed region. 2) The flare had the double-ribbon structure with the separation velocity of about 5 km/sec. 3) The filament in connection with the flare was located at the boundary of a large scale magnetic field with opposite polari...             本文对1980年10月15日产生在小黑子区的3级大耀斑作了详细的形态分析,,结果表明:1)耀斑无闪相,耀斑的最大强度为周围来扰区的2.4倍。2)耀斑有M带结构,双带的分离速度为5公里/秒。3)和耀斑有关的暗条位于大尺度磁场的极性分界线上,它在耀斑前和耀斑期间有明显变化,最终全部消失。4)耀斑的微波爆发增量小,上升下降缓慢,米波段有Ⅱ、Ⅲ、Ⅳ型爆发。5)耀斑的x射线辐射引起电离层2级骚扰(SLD)。耀斑无地磁暴对应。6)产生耀斑的活动区在日面存在3周,耀斑产生在活动区的衰亡阶段。以上结果基本与文献相同。 在本文的最后一节,对无黑子或小黑子区的耀斑形成作了简短的讨论,指出由日珥物质下落形成大耀斑所遇到的能量亏缺;日珥物质下落形成的激波,由于磁场的存在而强度削弱,磁场不能通过激波转化为辐射能;无黑子(或小黑子)区的耀斑的形成,在机理上可能与黑子区形成的耀斑类同。 文摘来源   << 更多相关文摘         相关查询: microwave burst spectrum sun microwave burst solar microwave burst microwave burst microwave type iii burst microwave type ⅲ burst microwave type ⅳ burst microwave type-ⅲ burst microwave combined type ⅲ burst sun-solar flare-microwave burst microwave generators  对查询结果不满意

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