Ripples and Rush-to-the-Poles in the photospheric magnetic field
Elena S. Vernova, Marta I. Tyasto, Dmitrii G. Baranov

TL;DR
This study analyzes solar magnetic field data to identify two types of magnetic flows, RTTP and ripples, revealing their characteristics, periodicities, and relationship with the solar cycle.
Contribution
It introduces the concept of ripples as a new type of magnetic flow between RTTP events, highlighting their periodicity and connection to the solar magnetic cycle.
Findings
RTTP flows drift from mid-latitudes to poles over 3 years.
Ripples have a period of about 1.1-1.3 years and occur between RTTP events.
Magnetic field amplitudes are higher when polar fields are positive.
Abstract
The distribution of magnetic fields of positive and negative polarities over the surface of the Sun was studied on the basis of synoptic maps presented by the NSO/Kitt Peak (1978-2016). To emphasize the contribution of weak fields the following transformation of synoptic maps was made: for each synoptic map only magnetic fields with modulus less than 5G (G) were left unchanged while larger or smaller fields were replaced by the corresponding threshold values +5G or G. Cyclic variations of the magnetic field polarity have been observed associated with two types of magnetic field flows in the photosphere. Rush-to-the-Poles (RTTP) appear near the maximum of solar activity and have the same sign as the following sunspots. The lifetime of RTTP is yrs, during which time they drift from latitudes - to the pole, causing the polarity change of the…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Astro and Planetary Science · Ionosphere and magnetosphere dynamics
