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We present a physical interpretation for the generation of circularpolarization resulting from the propagation of radiation through a magnetizedplasma in terms of a rotation measure gradient, or `Faraday wedges'. Criteriafor the observability of scintillation-induced circular polarization areidentified. Application of the theory to the circular polarization in pulsarsand compact extragalactic sources is discussed.Comment: 21 pages, 3 figures, ApJ, accepte

Scintillation‐induced Circular Polarization in Pulsars and Quasars