Hewish A
Cavendish Laboratory, Madingley Road, Cambridge CB3 0HE, United Kingdom.
Phys Rev E Stat Phys Plasmas Fluids Relat Interdiscip Topics. 2000 Aug;62(2 Pt B):3007. doi: 10.1103/physreve.62.3007.
Superluminally moving charge distributions of the type considered by Ardavan commonly occur inside waveguides and the radiation emitted by such sources is well known. The application of standard antenna theory shows that Ardavan has overestimated the intensity from typical pulsars by a factor exceeding 10(9).
阿尔达万所考虑的那种超光速移动电荷分布通常出现在波导内部,并且此类源发出的辐射是众所周知的。标准天线理论的应用表明,阿尔达万高估了典型脉冲星的辐射强度,高估因子超过10的9次方。