根据行星际闪烁(IPS)的双频互谱估计太阳风速度

USE TWO-FREQUENCY CO-SPECTRUM OF INTERPLANETARY SCINILLATION TO COMPUTE THE VELOCITY OF SOLAR WIND

本文讨论了观测频率为232MHz和327MHz时，利用互谱的方法估计太阳风速度的可能性、考虑路径积分效应，结果表明在17°≤ε≤50°范围内，对于几种可能的太阳风速度分布，由互谱所得结果与太阳风速度值差别小于15％．

The possibility of computing the velocity of solar wind by means of co-spectrumtechnique at two frequency 232 WHz and 327MHz is discussed in thes paper. Whenthe effect of integrahon is considered at the elongations 17°-50° with some possiblevelocity distribution, the derived results from co-spectrm tochnique indicate adeviation less than 15% from the velocity of solar wind.