New dynamo pattern revealed by solar helical magnetic fields

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. There are, however, two significant time-latitudinal domains in each cycle when the sign does briefly invert. Our findings shed new light on stellar and planetary dynamos and has yet to be included in the theory.

4 pages, 2 figures 0 tables. MNRAS Letters, accepted

References in corpus (3)

• Evolution and Distribution of Current Helicity in Full-Sun Simulations
• The distribution of current helicity at the solar surface at the beginning of the solar cycle
• Current Helicity and Twist as Two Indicators of The Mirror Asymmetry of solar Magnetic Fields

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