太阳射电爆发

太阳射电爆发中Spike辐射的准周期振荡

The quasi - periodic oscillation of spike radiation occurred in solar radio burst

1993年10月2日太阳射电爆发事件的证认和分析

Confirmation and Analysis of a Solar Radio Burst on 1993 October 2

1991年5月10日太阳射电爆发中Spike辐射的准周期振荡特征

The features of quasi - periodic oscillation of 1O May 1991 spike radiation

D.公布的米波射电大爆发资料，给出了毫秒级尖峰辐射的各种特征，总结出毫秒级尖峰辐射同Ⅲ型、Ⅱ型和Ⅳ型太阳射电爆发的关系，最后做出了相应的解释和讨论。

The relation between the millisecond spikes and the solar radio bursts of types ⅲ, ⅱ and ⅳ is also summarized . Finally , the corresponding explanation and discussion are presented .

太阳射电爆发准周期脉动的研究概况

Research resume of the quasi-periodic pulsation in solar radio burst

太阳射电爆发与高能质子加速过程

Solar Radio Bursts and Acceleration Processes of Energetic Protons

太阳射电爆发精细结构的特征提取和参数统计

Pattern Recognition and Parameter Statistics of Fine Structures in the Solar Radio Bursts

太阳射电爆发中纤维精细结构频漂率的计算

Frequency Drift Rate of Solar Radio Fiber Structures

第21、22周峰年太阳射电爆发中毫秒级精细结构的分析

An analysis of the millisecond fast fine structures of solar radio bursts during solar cycle 21,22

本文主要研究太阳射电爆发中纤维精细结构特征参数的计算。

This thesis mostly study the calculation of feature parameters of fiber fine structures in solar radio bursts .

由此，可以计算精细结构的特征参数，并进行统计分析，从而揭示太阳射电爆发的本质。

Finally the parameters of fine structures is calculated and analyzed so as to understand the physics of solar radio burst .

太阳射电爆发是太阳耀斑在无线电波段的一种表现，并相当敏感地反映了耀斑的能量释放过程。

Olar radio burst is a kind of manifestation of solar flare in radio wavelength band . It reflects sensitively the energy release process .

分米波毫秒级太阳射电爆发的几个形态发作早期脑电异常主要分快活动、慢活动及快慢混合活动三大类。

The early ictal EEG pattern were mainly classified into three groups of fast activities , slow activities and mixed activities according to its frequency characteristics .

1998年4月15日太阳射电爆发同时在这两台频谱仪上记录到。这个事件在时间和频率上显示了丰富的幅度和结构的变化。

The solar radio burst was recorded at the same time by the two spectrometers on April 15, 1998.Some new interesting results are found , suchas a pair of microwave type ⅲ bursts and rich fast fine structures .

北京天文台密云观测站（工作频率146兆赫）于1972年8月得到了太阳射电爆发以及同238活动区（McMath11976）相连系的Ⅰ型源的一些观测结果。

Some results of measurements made in August 1972 of the solar radio bursts and the Type-I source associated with the active region 238 ( MeMath 11976 ) have been obtained at Miyun station , Peking Observatory ( working frequency 146 MHz ) .

太阳射电微波爆发谱与HXR的统计研究

The statistics investigation on solar microwave bursts and HXR bursts

1990年7月30日太阳射电大爆发中的脉动现象

Pulsation phenomena in the solar burst on July 30 , 1990

太阳射电微波爆发及其精细结构研究进展

Progress of Solar Radio Microwave Bursts and Fine Structures

太阳射电微波爆发的频谱分析

A spectral analysis of the Solar Radio Microwave Burst on 1 April 1981

太阳射电米波爆发与日冕物质喷射

Solar Radio Meter Burst and Coronal Mass Ejections

一个太阳微波射电爆发中的快速脉动现象

Fast Pulsative Phenomena in Solar Microwave Burst

太阳米波射电爆发是活动区上空日冕中的现象，与太阳耀斑有密切关系。

Solar radio burst on metric wavelengths , which is associated with solar flare , is a phenomenon in the corona above solar active regions .

太阳射电微波爆发携带着爆发源区的物理环境及辐射机制等诸多重要信息。

The complicated radio spectrum detected in solar radio bursts contain a lot of important information on their source regions including physical environment and emission mechanisms .

太阳射电IV型爆发U形谱的产生机制

The mechanism of the U-shaped spectrum of the type IV solar radio bursts

太阳射电IV型爆发及伴随现象与白光耀斑的关系

The Relation between Type IV Solar Radio Bursts and Associated Phenomena and White Light Flares

太阳射电Ⅰ型爆发频谱观测和处理程序设计

Program Design for Spectral Observations of Type ⅰ Solar Radio Bursts

日冕和行星际空间中的太阳射电Ⅱ型爆发

Solar Radio Type ⅱ Burst in the Corona and Interplanetary Medium

电离层D层突然骚扰与太阳耀斑微波射电爆发的关系

Relationship between Sudden Ionospheric Disturbances in D Layer and Solar Microwave Bursts

由束流不稳定性直接激发电磁波来解释太阳射电Ⅲ型爆发

The Direct Excitation of Electromagnetic Waves by Beam Instabilities and Explanation for Solar Type - ⅲ Radio Bursts

太阳质子事件与射电爆发和软X射线耀斑间的关系

Relationship between solar proton events and solar radio bursts or soft X-ray flares