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对《聚焦的、非球对称衰减电磁辐射脉冲的产生》的评论I

Comment I on "Generation of focused, nonspherically decaying pulses of electromagnetic radiation".

作者信息

Hewish A

机构信息

Cavendish Laboratory, Madingley Road, Cambridge CB3 0HE, United Kingdom.

出版信息

Phys Rev E Stat Phys Plasmas Fluids Relat Interdiscip Topics. 2000 Aug;62(2 Pt B):3007. doi: 10.1103/physreve.62.3007.

DOI:10.1103/physreve.62.3007
PMID:11088797
Abstract

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).

摘要

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。

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