A study of the fine structures superimposed on solar bursts in the 2.6-3.8 GHz frequency band

Ning Zong-jun; Fu Qi-jun; Lu Quan-kang

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A study of the fine structures superimposed on solar bursts in the 2.6-3.8 GHz frequency band

机译：对2.6-3.8 GHz频带上太阳爆发叠加的精细结构的研究

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摘要

Microwave type III bursts and microwave spikes superimposed on solar bursts observed by Beijing Astronomical Observatory (BAO) are studied in this paper. The bursts and spikes are closely related and together they make up fine structure clusters; but the time resolution of the instrument plays an important role in their relation.

机译：本文研究了北京天文台（BAO）观测到的Ⅲ类微波爆发和叠加在太阳爆发上的微波尖峰。突发和尖峰密切相关，它们共同构成了精细的结构簇。但是仪器的时间分辨率在它们之间的关系中起着重要作用。

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《Chinese Astronomy and Astrophysics》 |2000年第2期|共7页
作者
Ning Zong-jun; Fu Qi-jun; Lu Quan-kang;
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正文语种 eng
中图分类天文学;
关键词
solar microwave bursts; fine structures;

机译：太阳微波爆发;精细结构;

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专利

1. A study of the fine structures superimposed on solar bursts in the 2.6-3.8 GHz frequency band [J] . Ning Zong-jun, Fu Qi-jun, Lu Quan-kang Chinese Astronomy and Astrophysics . 2000,第2期

机译：对2.6-3.8 GHz频带上太阳爆发叠加的精细结构的研究
2. 60-GHz oxygen band: precise of fine-structure lines, broadening and central frequencies absolute absorption profile at atmospheric pressure, and revision of mixing coefficients [J] . Tretyakov MY, Koshelev MA, Dorovskikh VV, Journal of Molecular Spectroscopy . 2005,第1期

机译：60 GHz氧气带：精细结构线的精确度，大气压下的展宽和中心频率绝对吸收曲线，以及混合系数的修正
3. A Study of Solar Radio Bursts with Fine Structures during Flare/CME Events [J] . J. Huang, Y.H. Yan, Y.Y. Liu Solar physics . 2009,第1a2期

机译：耀斑/ CME事件中具有精细结构的太阳射电爆发的研究
4. OCCURRENCES OF DIFFERENT TYPES OF 0.8-2.0 GHZ SOLAR RADIO BURSTS AND FINE STRUCTURES DURING THE SOLAR CYCLE [C] . K. Jiricka, M. Karlicky, H. Meszarosova, Solar cycle and space weather euroconference . 2002

机译：在太阳循环期间出现不同类型的0.8-2.0 GHz太阳能无线电突发和细结构
5. Perceptual weighting of the envelope and fine structure across frequency bands during continuous and interrupted speech. [D] . Fogerty, Daniel. 2010

机译：在连续和间断语音期间，整个频带的包络和精细结构的感知加权。
6. Imaging spectroscopy of solar radio burst fine structures [O] . E. P. Kontar, S. Yu, A. A. Kuznetsov, -1

机译：太阳射电爆发细微结构的成像光谱
7. Occurrence of Solar Radio Burst Fine Structures in 1–7.6 GHz Range Associated with CME Events [O] . Yihua Yan, Yuying Liu, Zhijun Chen, 2004

机译：在与CME事件相关联的1-7.6 GHz范围内发生太阳能无线电突发细结构
8. New Class of Solar Burst with mm-Wave Emission But Only at the Highest Frequency (90 Ghz) [R] . Kaufmann, P., Correia, E., Costa, J. E. R., 1984

机译：具有毫米波发射的新型太阳能爆破但仅在最高频率（90 Ghz）

A study of the fine structures superimposed on solar bursts in the 2.6-3.8 GHz frequency band

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