2019
DOI: 10.48550/arxiv.1912.13223
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Magnetic field dependence of bipolar magnetic region tilts on the Sun: Indication of tilt quenching

Bibhuti Kumar Jha,
Bidya Binay Karak,
Sudip Mandal
et al.

Abstract: The tilt of bipolar magnetic region (BMR) is crucial in the Babcock-Leighton process for the generation of the poloidal magnetic field in Sun. Based on the thin flux tube model of the BMR formation, the tilt is believed to be caused by the Coriolis force acting on the rising flux tube of the strong toroidal magnetic field from the base of the convection zone (BCZ). We analyze the magnetic field dependence of BMR tilts using the magnetograms of Michelson Doppler Imager (MDI) (1996)(1997)(1998)(1999)(2000)(2001)… Show more

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