Divergence:
A maximum of converegnce is found below the cloudiness of the Convergence Line, reach from very low troposphere up to 600 hPa. The values are quite low. This is due to the coarse resolution of the globle model. LAM models can give better correlation and show more intensive convergence.
Vertical Motion (Omega):
Upward motion is found at all levels at the Convergence Line. This is more than usual expected extend where upward motion is found reaching only a little bit higher than convergence. As mentioned before LAM fields could show the structure more precisely.