This phenomenon is transported by a meridional flow and by differential rotation, and as this phenomenon is transported outward from its origin by wind it forms a structure known as a Parker spiral.
One of the most extensive maps of this phenomenon has been produced using Zeeman interferometry by the Michelson Doppler Imager aboard the SOHO mission, while another method for mapping it relies on the Hanle effect. Some distance from its origin, this phenomenon divides into "open" and "closed" regions, and it undergoes large-scale adjustments on a timescale of days as a result of the formation and dissipation of supergranules. This phenomenon is transported by a meridional flow and by differential rotation, and as this phenomenon is transported outward from its origin by wind it forms a structure known as a Parker spiral. This is responsible for the dark color of objects whose polarity undergoes shifts in 11-year cycles. FTP, identify this phenomenon, a field induced by the dynamo process inside the star which we orbit.
One of the most extensive maps of this phenomenon has been produced using Zeeman interferometry by the Michelson Doppler Imager aboard the SOHO mission, while another method for mapping it relies on the Hanle effect.
{solar magnetic} field [or the {magnetic} field of the {sun}, prompt on any sort of partial answer]