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Poynting's theorem and time-harmonic radiators

机译:Poynting的定理和时间谐波散热器

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An important parameter of any antenna is the ratio of standing reactive energy stored about the antenna to the radiated power; by definition, quality factor Q is /spl omega/ times that ratio. Q is often inversely proportional to the operational bandwidth of the antenna. Extensive experience and electromagnetic theory arguments based upon Q seem to agree that an efficient antenna must be about a half wavelength long in at least one dimension. But is this a general property of radiation fields, or is it due to an inadequate understanding on our part? Can the size limitations be mitigated or even bypassed? In this paper we re-examine the fundamentals of radiating fields and conclude that there is a significant special case that has not been adequately examined previously. We examine it and conclude that errors of omission are made in previous analyses, and significant improvements in the operation of small antennas may be possible. The complex Poynting vector is derived from the time-domain equations. Using it there are two types of radiation fields that have convenient solutions, and these are presented.
机译:任何天线的一个重要参数是将天线存储到辐射动力的站立反应能量的比率;根据定义,质量因子Q为/ SPL omega /倍。 Q通常与天线的操作带宽成反比。基于Q的广泛体验和电磁理论争论似乎同意至少一个维度在至少一个维度中必须长度为大波长长度。但这是辐射领域的一般财产,还是由于我们的理解不足?尺寸限制是否可以减轻甚至绕过?在本文中,我们重新研究了辐射领域的基本原理,并得出结论,尚未以前审查过重大的特殊情况。我们检查它并得出结论,在先前的分析中进行遗漏的误差,并且可以进行显着改善小天线的操作。复杂的Poynting载体来自时域方程。使用它有两种类型的辐射场,具有方便的解决方案,这些辐射场呈现。

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