Fig. 1.
Two-component model. Linearly polarized flux density is shown with solid lines, and EVPA is shown with dashed lines. Flux density and time are in arbitrary units. Φ is the EVPA rotation across the burst and Ψ is the EVPA difference (jet – burst) at time t = 0. In this example, Φ = 70°, Ψ = 75°, and R = ratio of peak burst flux to jet flux = 1.3.
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