  An extended XMM-Newton observation of the luminous narrow line Seyfert galaxy
PG 1211+143 in 2014 has revealed a more complex high velocity wind, with
components distinguished in velocity, ionization level, and column density.
Here we report soft x-ray emission and absorption features from the ionized
outflow, finding counterparts of both high velocity components, v ~ 0.129c and
v ~ 0.066c, recently identified in the highly ionized Fe K absorption spectrum.
The lower ionization of the co-moving soft x-ray absorbers imply a distribution
of higher density clouds embedded in the main outflow, while much higher column
densities for the same flow component in the hard x-ray spectra suggest
differing sight lines to the continuum x-ray source.
