Abstract

In this letter, the distribution of the Rice factor $(K)$ is experimentally evaluated within the mode stirred reverberating chamber (RC) of the Universita Degli Studi di Napoli Parthenope, formerly Istituto Universitario Navale (IUN), Naples, Italy. The experimental distribution obtained for different $K$ -values is contrasted with a reference Nakagami- $m$ distribution. To generate different $K$ -values, the same RC configuration is adopted with a nonstationary receiving antenna position, i.e., the receiving antenna is placed on a rotating table. Experimental results confirm the soundness of the approach and demonstrate that K distribution well fits the reference Nagakami- $m$ model.

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