  Periodic outbursts are observed in several changing-look (CL) active galactic
nuclei (AGNs). \citet{sniegowska_possible_2020} suggested a model to explain
the repeating CL in these AGNs, where the periodic outbursts are triggered in a
narrow unstable zone between an inner ADAF and outer thin disk. In this work,
we intend to investigate the effects of large-scale magnetic fields on the
limit cycle behaviors of CL AGNs. The winds driven by magnetic fields can
significantly change the structure of thin disk by taking away the angular
momentum and energy of the disk. It is found that the period of outburst in
repeating CL AGNs can be substantially reduced by the magnetic fields.
Conversely, if we keep the period unchanged, the outburst intensity can be
raised for several times. These results can help to explain the observational
properties of multiple CL AGNs. Besides the magnetic fields, the effects of
transition radius $R_{\rm tr}$, the width of transition zone $\Delta R$ and
Shakura-Sunyaev parameter $\alpha$ are also explored in this work.
