Evolution of stellar properties for models of masses 1 M_⊙ (dark blue), 1.3 M_⊙ (light blue), 1.6 M_⊙ (green), 1.9 M_⊙ (magenta), 2.2 M_⊙ (orange), and 2.5 M_⊙ (red) computed with MESA, as a function of ν_max (in log scale, inverted axis), from ν_max = 300 μHz up to ν_max = 20 μHz. Plain lines represent the evolution along the RGB while dots indicate median values on the HB. Models with masses of 1.3 M_⊙ and 1.6 M_⊙, representative of the median masses for LM and IM stars on the RGB, respectively, are highlighted in bold. The vertical dashed lines indicate ν_max = 100 μHz. Left: Convective turnover timescale. Right: Rossby number.