\label{tab:tab1}
\label{clumps}
| M | Zone | \({\mathrm{H}_{\mathrm{P}}}\) | \({\langle{{v}_{c}}\rangle}\) | \(\Delta M_{\rm conv}\)1 | \(\Delta M_{\rm top}\)2 | \(N_{\rm cells}\)3 | \(\tau_{\rm turn}\)4 | \(\tau_{\rm conv}\)5 | \( \dot{M}\) |
| \({\,\mathrm{M}_\odot}\) | \({\,{\rm R}_\odot}\) | km s\(^{-1}\) | \({\,\mathrm{M}_\odot}\) | \({\,\mathrm{M}_\odot}\) | days | days | \({\,\mathrm{M}_\odot}\rm{ yr}^{-1}\) | ||
| 20 | He | 0.025 | 0.08 | \(7.6\times10^{-9}\) | \(1.9\times10^{-9}\) | \(1.8\times10^{5}\) | 2.5 | 38 | \(7.3\times10^{-8} \) |
| 20 | Fe | 0.08 | 2.40 | \(3.6\times10^{-6}\) | \(5.8\times10^{-7}\) | \(1.8\times10^{4}\) | 0.25 | 18250 | \(7.3\times10^{-8}\) |
| 60 | Fe | 0.24 | 2.25 | \(1.6\times10^{-5}\) | \(9.8\times10^{-7}\) | \(8.5\times10^{3}\) | 0.83 | 1570 | \(3.7\times10^{-6}\) |
Mass contained in the convective region.↩
Mass in the radiative layer between the stellar surface and the upper boundary of the convective zone.↩
Expected number of convective cells, \(N_{\rm cells}:= (R_{\star}/H_{\rm P})^2\).↩
Convective turnover time, \(\tau_{\rm turn}:= H_{\rm P}/{\langle{{v}_{c}}\rangle}\).↩
Time that a piece of stellar material spends inside a convective region, \(\tau_{\rm conv}:= \Delta M_{\rm conv}/\dot M\).↩