Fig. 3

image

Longterm 146 MHz radio lightcurve of CR Dra in total intensity SI (top panel), circular polarisation SV (middle panel), and the ratio |SVSI|. Only positive Stokes V emission is detected, implying we observe only left-hand circularly polarised emission from CR Dra. Uncertainties represent 1σ and are only shown if larger than the symbol size. The ratio |SVSI| is plotted if the corresponding signal-to-noise ratio of CR Dra is ≥3σ in both Stokes I and Stokes V emission. We show 3σ upperlimits for |SVSI| if the emission in Stokes I is ≥ 3σ but < 3σ in Stokes V.

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