Notes. Table columns: total mass M, effective radius R_eff, column density N_H2, number density n_H2, non-thermal velocity dispersion ΔV_NT, corrected non-thermal velocity dispersion $\Delta V_{\text{NT}}^{*}$, position angle of major axis ϕ_PA, circular mean of the magnetic held orientations ϕ_B, circular angular dispersion of the magnetic held orientations σ_ϕ, ratio of turbulent to large-scale magnetic held components $\frac{\langle B_t^2\rangle }{\langle B_0^2\rangle }$, plane-of-sky magnetic held strength B_POS, gravitational energy density u_G, magnetic held pressure P_B, and turbulent pressure P_T. The uncertainties of M and N_H2, related quantities are propagated from the errors of the measured intensity, temperature and dust opacity as described in Section 4.2.^(a) Line-width from NH₃ (1.1) line (Lu et al. 2014). ^(b)Due to the lack of a large enough number of polarization segments and the uniformity of the magnetic held within these clumps, the best-fit of structure function failed. ^(c)Note the angular dispersion of the magnetic held orientation for SDC18-N-1 and SDC18-N-3 are calculated using polarization segments outside of the defined core boundaries (see Section 4.2).