Radial, azimuthal and meridional components of the large-scale magnetic field at the surface of Gl 205 for the four subsets of data defined in Sect. 5.2. From top to bottom, the rows show the results for Seasons S₁ (September-December 2019), S₂ (August-October 2020), S₃ (August–September 2021), and S₄ (November 2021–January 2022). Each panel is a flattened polar view of the stellar surface. The circles indicate the equator (black solid line) and the –30, 30 and 60° parallels (dashed lines) and the ticks around the star mark the spectropolarimetric observations in unit of stellar rotation phase. The color bar depicts the magnetic flux in Gauss.