射电辐射

本文结果表明，γ射线和射电辐射都来自喷流，γ射线很可能产生于同步自康普顿（SSC）过程。

Our result shows that the γ - rays are associated with the radio emission from the jet , and that the γ - ray emission is likely to have come from the synchrotron self-Compton model ( SSC ) process in this case .

太阳射电辐射的自调制模型

A self-modulation model of solar radio emission

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

1981年4月1日大耀斑的X射线、可见光和射电辐射的观测研究

X-Ray , H_ α, and Radio Observational Study of the 4N / X2.3 Flare of April 1,1981

CME影响下L1点附近等离子体及共生微波爆发的射电辐射机制研究

Study on the Radiation Mechanism of Plasmas Near L1 Point Affected by CMEs and the Associated Microwave Bursts

用离散相关函数方法分析Blazar天体的γ射线和射电辐射的相关性

Analysis of the correlation between γ - ray and radio emissions from γ - ray loud Blazar using the discrete correlation function

大幅度快速光变、高偏振、整个电磁波段的非热连续辐射及致密的射电辐射是blazar天体的主要特征，blazar天体的统一与演化是blazar天体研究的重要内容。

Blazar is mainly characterized by rapid variability with a large amplitude , high polarization , compact radio radiation , and nonthermal radiation in the electromagnetic wave from radio bands to gamma rays . An important research aspect for the blazar is the unification and evolution of blazar .

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

黑洞自转和类星体喷流射电辐射的相关性

On the Correlation of Black Hole Spin and Radio Jet Radiation of Quasars

脉冲星的射电辐射特性和磁倾角

Radio radiation characteristics of pulsars and magnetic dipole angle

太阳耀斑的厘米波和分米波射电辐射

Centimeter and Decimeter Wavelength Emissions from Solar Flares

GPS/LEO掩星方法中的电离层延迟量对太阳射电辐射流量的响应

Impact of Solar Radio Flux on Ionospheric Phase Delay in GPS / LEO Occultation Methodology

而γ射线辐射流量的最小值和射电辐射流量之间没有相关性。

And there are no correlation between γ - ray emission and radio emission in low state .

γ射线辐射与射电辐射谱指数之间也有相关性存在。

In addition , there is a correlation between the γ - ray and radio spectral index .

发现缺脉冲现象显著的脉冲星分布在射电辐射的截止线附近，组成一条近于和截止线平行的直线。

The pulsars with long pulse nulling distribute near the radio cut-off line and constitute a line nearly parallel to the cut-off line .

然后对有关射电辐射机制、传播的理论作了一个简要的回顾。

Then , an overview of the theory of radio emission mechanisms and the propagation of radio emission in solar coronal was done .

简要地评述了活动星系核中吸积盘与喷流存在内在联系的观测证据，及中央黑洞与活动星系核的射电辐射特征的关系。

The observational evidence on the disk-jet connection in active galactic nuclei and the correlation between the central black holes and their radio properties are summarized .

主要结果如下：对于最小值而言，γ射线辐射与射电辐射流量密度之间没有相关性存在；

Our results are as follows . For minimum γ - ray data , there is no correlation between the γ - ray and radio flux density ;

最后研究了脉冲星表面磁层中的磁化等离子体与在其间产生并传播的射电辐射的相互作用修正了射电辐射谱的引力红移。

Finally studied in how does the magnetization plasma in the magnetosphere of pulsars cause the spectrum of the radio radiation shifting and the gravitational redshift of the pulsar radiation is corrected .

本文对81颗脉冲星作了统计分析，所得结果似支持射电辐射产生于光速圆柱附近的看法。

The results of statistical analyses of radio luminosity of 81 pulsars obtained in this paper are likely in favor of the version that the radio radiation is emitted from the region near the light cylinder .

太阳空间观测揭示出太阳的高能电子、高能质子发射以及γ射线爆发。证实了有关的太阳射电辐射理论、揭示出太阳耀斑中的核反应。

The ejection of energetic electrons and protons , and γ - ray burst are revealed by solar space observations , which have confirmed some related theories of solar radio emission and uncovered the nuclear reaction in flares .

澳大利亚研究者最近所作的一项为期3年的研究显示手机的射电辐射不会引发老鼠体内肿瘤的生长，因此可能也不会对人造成这样的伤害。

A recent one carried out by Australian researchers over a three-year eriod showed that radio emissions from mobile phones did not trigger the growth of tumors in mice , and therefore probably did not do so in humans either .

正常星系的射电连续辐射及HI辐射

Radio Continuum Radiation and HI Radiation of Normal Galaxies

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

太阳射电SVC辐射模型

A model of radiation for solar radio SVC

本文综述了近年来世界上各大天文台站对正常星系的射电连续辐射和HI辐射的观测及研究。

The observations and study of radio continuum radiation and HI radiation of normal galaxies carried out by the main observatories in the world in recent years is described .

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 .

而当哈雷彗星第二次过近地点时期，利用M24微机数据采集系统，对该彗星进行追踪观测。得到在此期间哈雷彗星21厘米射电连续辐射强度的上限为2.22Jy（5σ）。

The upper limit of the intensity of the 21-cm wavelength continuous radiation of Halley 's Comet is 2.22 Jy ( 5 σ) .

太阳射电尖峰辐射的电子回旋脉泽增长率

Electron Cyclotron Maser Growth Rates of Solar Radio Spike Radiation