MICROWAVE ABSORPTION IN THIN CONDUCTORS OF FINITE LENGTH
Abstract
Subject and Purpose. Many of the currently known calculations of the strong absorption of electromagnetic radiation in conductors whose diameter is several hundred times smaller than the radiation wavelength proceed from the physical effects accompanying interaction of an electromagnetic wave with an infinitely long conductor. However, antenna theory shows that resonant phenomena in finite-seized conductors can significantly enhance or suppress the interaction of conductors with electromagnetic radiation. This paper examines the interaction of a thin conductor of finite length with a plane, linearly polarized electromagnetic wave, focusing in particular on the amount of energy absorption and the effects due to the length of the conductor.
Methods and Methodology. The solution to the integral equation for the current through a thin conductor has been sought for in an asymptotic averaging technique. Using the Joule-Lenz law and calculating the conductor's resistance, the power absorbed by the conductor is calculated. This allows determining the absorption efficiency factor for the radiation incident on a conductor of finite length.
Results. The amount of the electromagnetic radiation energy absorbed within a thin conductor has been studied in dependence on the conductor’s finite length. As has been found, when the length of the conductor is close to half the radiation wavelength, else to a multiple of that value, the absorption increases by tens of times compared to the value demonstrated by an infinitely long conductor.
Conclusions. The results permit clarifying the previously existing understanding of the interaction of microwave radiation with thin conducting structures and can find application in the development of compact absorbing loads, field shielding elements and structures for microwave energy transmission.
Keywords: microwave radiation, thin conductors, energy absorption, resonance effects, electromagnetic interaction
Manuscript submitted 23.06.2026
Radio phys. radio astron. 2026, 31(3): 190-198
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