  We present the analysis of three kinds of oscillating behavior using
multi-wavelength observations of the 10 November 2013 (SOL2013-11-10T05:14)
circular-ribbon flare. This event is a typical circular-ribbon flare with an
outer spine structure and homologous jets. We found three kinds of oscillations
(or perturbations): i) flux oscillation (or QPP) with a dominant period of
about 20 seconds in X-ray, EUV, and microwave emissions, ii) periodic jets with
an intermittent cadence of around 72 seconds, iii) an outer loop perturbing
half a cycle with a duration of about 168 seconds. Similar to the periodic jets
that could be produced by a nonthermal process, like repeated magnetic
reconnection, the flare QPP detected in the thermal emissions could have the
same origin as the oscillation seen in the nonthermal emissions. The outer-loop
perturbation is possibly triggered by a blast wave driven by the
circular-ribbon flare, or it might be modulated by the sausage wave or the slow
magnetoacoustic wave. The results obtained provide data for further numerical
studies on the physical origin of the flare oscillations.
