New dynamo pattern revealed by solar helical magnetic fields
Hongqi Zhang, T. Sakurai, A. Pevtsov, Yu Gao, Haiqing Xu, D. D., Sokoloff, K. Kuzanyan

TL;DR
This study reports the first direct measurement of the mirror asymmetry in solar magnetic fields, revealing new patterns in solar helicity that challenge existing dynamo theories and enhance understanding of magnetic field generation.
Contribution
The paper provides the first observational evidence of persistent hemispheric helicity patterns and their brief inversions, offering new insights into solar and stellar dynamo mechanisms.
Findings
Hemispheric helicity patterns propagate equatorward.
Helicity sign remains consistent across cycles, with brief inversions.
Results challenge existing dynamo models and suggest new theoretical considerations.
Abstract
Previously unobservable mirror asymmetry of the solar magnetic field -- a key ingredient of the dynamo mechanism which is believed to drive the 11-year activity cycle -- has now been measured. This was achieved through systematic monitoring of solar active regions carried out for more than 20 years at observatories in Mees, Huairou, and Mitaka. In this paper we report on detailed analysis of vector magnetic field data, obtained at Huairou Solar Observing Station in China. Electric current helicity (the product of current and magnetic field component in the same direction) was estimated from the data and a latitude-time plot of solar helicity during the last two solar cycles has been produced. We find that like sunspots helicity patterns propagate equatorwards but unlike sunspot polarity helicity in each solar hemisphere does not change sign from cycle to cycle - confirming the theory.…
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