  The process of the Sun's polar field cancellation reversal commences with the
emergence of new cycle Hale's polarity active regions. Once the Sun undergoes
polarity reversal, typically occurring near the peak of solar activity, it
begins the process of accumulating the seed field for the forthcoming solar
cycle. In recent years, the Advective Flux Transport (AFT) model has proven
highly effective in forecasting the progression of polar fields by leveraging
observations of surface flows and magnetic flux emergence. In this study, we
make use of the predictive capability of the AFT model to simulate the
evolution of the polar fields and estimate the timing of the Solar Cycle 25
polarity reversal in both hemispheres of the Sun. We use the statistical
properties of active regions along with Solar Cycle~13, which closely resembles
the current solar cycle (Cycle~25), to generate synthetic active regions in
order to simulate future magnetic flux emergence in AFT to predict the
evolution of the polar field. Based on our simulations, we anticipate that the
Northern hemisphere of the Sun will undergo a polarity reversal between June
2024 and November 2024, with the center of our distribution at August 2024. In
the Southern hemisphere, we anticipate a polarity reversal between November
2024 and July 2025, centered around February 2025. Additionally, assuming that
the reversal of the axial dipole moment coincides with the peak of the solar
cycle, our findings indicate that Cycle 25 is expected to peak in 2024 (likely
between April to August 2024).
