射电流量

大耀斑爆发的Hα初始亮点，双带出现，环系形成，亮物质抛射和吸收冕珥等现象同3.2cm射电流量的变化在时间上有较好的对应关系。

During the major flare , the two-ribbon appearance , loop system formation , mass ejections and their flows back to the chromosphere had a good correspondance in time to the peaks of the 3.2 cm radio flux curve .

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

射电流量变化极大，显示出无规则爆发。

The radio flux is extremely variable , exhibiting erratic outbursts .

从10.7cm射电流量月平均变化说明了太阳活动的浑沌行为。

The predictable time scale for the monthly mean variations of the 10.7 cm radio flux is also discussed .

极大的射电流量同极小的角经集于一身，意味着这些发射源有难以置信的高表面亮度。

The combination of very large radio flux and exceedingly small angular size means that the sources have a fantastic surface brightness .

本文阐述了在二十一太阳周期上升相期间太阳黑子、钙谱斑、2800MHz射电流量和太阳耀斑、质子耀斑、质子事件的活动情况。

The activities of sunspots , calcium plages , 2800 MHz flux , solar flares and proton events during the rising phase of Cycle 21 arc expounded in this paper .

检波采用平方律检波器，只有在采用平方律检波器的前提下，接收记录与射电流量密度之间的线性关系才存在。

The square-law detector is used for detection , because only when the square-law detector is used , the linear relationship between the received record and the radio flow density exists .

对于双射电子源类星体，根据两子源射电流量之比以及射电光度演化规律等，可以推得子源相对于光学母体的分离速度。

For QSO with double radio components , the separation velocity of radio com - ponents with respect to the optical parent body can be derived from the radio flux ratio of the two components and the evolution law of radio luminosity .

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 .

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 ;

在这个样本所包括的37个IRAS星系中，探测到19个源的射电发射，获得了它们的射电参数，如峰值位置，射电流量等。

Radio emission was detected from 19 sources in the 37 IRAS galaxy sample . The radio parameters , for example , peak position , radio flux , etc.