Image Details
Caption: Figure 2.
Latitude profiles of changes in meridional flow (δUθ, in black) and zonal flow (δUϕ, in pink), averaged over 1 yr around the cycle 24 maximum, for depths 0.99 R⊙ (solid) and 0.95 R⊙ (dashed) in the top panel. The same in the radial gradient of rotation, ﹩\delta ({\rm{\partial }}\,{\rm{log}}\,{\rm{\Omega }}/{\rm{\partial }}\,{\rm{log}}\,r)﹩, along with the longitudinally averaged unsigned magnetic field (right y-axis), is shown in the lower panel. The error bars shown represent errors estimated in the inversion method (see Section 4.1 for details).
© 2025. The Author(s). Published by the American Astronomical Society.