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The tilt of the bipolar magnetic region (BMR) is crucial in theBabcock-Leighton process for the generation of the poloidal magnetic field inthe Sun. We extend the work of Jha et al. (2020) and analyze the recentlyreported tracked BMR catalogue based on AutoTAB Sreedevi et al. (2023) fromMichelson Doppler Imager (1996-2011) and Helioseismic and Magnetic Imager(2010-2018). Using the tracked information of BMRs based on AutoTAB, we confirmthat the distribution of bmax reported by Jha et al. (2020) is not because ofthe BMRs are picked multiple times at the different phases of their evolutioninstead it is also present if we consider each BMRs only once. Moreover, wefind that the slope of Joy's law initially increases slowly with the increaseof bmax. However, when bmax>2.5 kG, gamma_0 decreases. The decrease of observed$gamma_0$ with bmax provides a hint to a nonlinear tilt quenching in theBabcock-Leighton process.

Exploring the Quenching of Bipolar Magnetic Region Tilts using AutoTAB