太阳射电

发生在米波段的太阳射电辐射

Solar Radio Radiation Events Occurred in the Meter Waver Band

太阳射电辐射的第四种成份&太阳射电快变分量

The Fourth Component of the Solar Radio Radiation & the Rapidly Varing Component

太阳射电辐射事件与Hα耀斑的相关分析

The Correlation Analysis On the Solar Radiation Events and H α Flares

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

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

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

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

太阳射电毫秒Spike辐射窄带宽的理论探讨

A theoretical study on the narrow bandwidth of the solar radio millisecond spike radiation

双极黑子活动区中太阳射电SVC辐射

Solar radio SVC radiation in an active region of bipolar sunspot

PIN调制器在太阳射电快速记录系统中的运用和性能检测

The Application and Test on the Principal Performance of the Solar Radio Fast Recording System at the PIN Modulator

太阳射电SVC辐射模型

A model of radiation for solar radio SVC

根据这个理论模型，本文着重研究了太阳射电毫秒Spike辐射的频带宽度问题。

On the basis of the above model , we have emphatically studied the bandwidth of the solar radio millisecond 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 .

一般认为，Langmuir波转换为电磁波是太阳射电Ⅲ型暴的重要机制，由电子束流不稳定性可以很容易的激发Langmuir波。

Langmuir waves converted into electromagnetic radiation is an important mechanism of solar type ⅲ bursts . Langmuir waves can be easily excited by electron beam instability .

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

建议不仅是太阳射电、宇宙射电的相关课题和设备亦应注意配备HTR技术。

We suggest that the HTR technique should be engaged not only for the solar radio observational equipments but also for the cosmic subjects concerned .

13.7m抛物面天线增益测量和太阳射电流量密度定标

Gain Measurement of a 13.7m Paraboloid Antenna and the Calibration of Solar Radio Flux Density

USAF太阳射电全球巡视网及其第21太阳活动周U-型谱预报精度的检验

The Solar Radio Patrol Network of USAF and the Examination of Prediction Accuracy of the U-Shaped Radio Spectrum for Cycle 21

太阳射电频谱日像仪（CSRH）馈源的设计分析和性能测试

Feed Designing Analysis and Performance Testing for the Solar Spectral Radio Heliograph

微波Ⅲ型爆发在1-2GHz太阳射电快速频谱仪上的观测

Observation of Microwave Type ⅲ Bursts at 1-2 GHz

太阳射电尖峰辐射（spike）的窄频带是一个具有特征性的参数，不但可从它计算出Spike辐射源区的小尺度结构，而且观测结果与Spike辐射理论可相互验证。

The narrow bandwidth of a solar radio spike is a characteristic parameter . Using this spike bandwidth not only the small-scale structure of spike source dimension can be calculated but also the theory of spike emission can be checked with the observations .

1-2GHz太阳射电动态频谱仪

A Solar Radio Dynamic Spectrometer at 1-2 GHz

本文分析研究了22GHz频率上高分辨率（～4′）的太阳射电观测资料。

In this paper we analysed the observational data of solar radio emission at 22 GHz with a resolution of - 4 ' .

在磁拱底部非线性等离子体密度波传播期间，损失锥分布的反射电子驱动着电子回旋maser不稳定性的增长，激励出二次谐频波模，支配着太阳射电毫秒Spike辐射。

The reflected electrons of a loss-cone distribution can drive the electron cyclotron maser instability when a nonlinear density wave travells through the bottom part of the magnetic loop . The maser instability will excite the second harmonic O-mode and X-mode to dominate the solar radio millisecond spike radiation .

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

光电二极管阵在太阳射电频谱研究中的应用

An Application of Photodiode Array in the Solar Radio Spectral Research

太阳射电常规观测定标自动化的实现

Realization of the Scaling Automation for the Solar Radio Routine Observation

用于太阳射电观测的宽频带米波菱形天线

A Wide Band Meter-wave Rhombic Antenna Used for Solar Radio Observation

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

太阳射电米波准周期振荡事件分析

Analysis of the Quasi-periodically Oscillatory Event of Solar Radio Metric Wave