  The unusual behavior of the spectral lines of NGC5548 during the STORM
campaign demonstrated a missing piece in the structure of AGNs. For a two-month
period in the middle of the campaign, the spectral lines showed a deficit in
flux and a reduced response to the variations of the UV continuum. This was the
first time that this behavior was unequivocally observed in an AGN. Our
previous papers explained this as being due to a variable disk-wind which acts
as a shield and alters the SED. Here we use Cloudy to create an atlas of
photoionization models for a variety of disk-winds to study their effects on
the SED. We show that the winds have three different cases: Case 1 winds are
transparent, fully ionized and have minimal effects on the intrinsic SED,
although they can produce some line emission, especially HeIIor FeK{\alpha}. We
propose that this is the situation in most of the AGNs. Case 2 winds have a
He++-He+ionization-front, block part of the XUV continuum but transmit much of
the Lyman continuum. They lead to the observed abnormal behavior. Case 3 winds
have H+ionization-front and block much of the Lyman continuum. The results show
that the presence of the winds has important effects on the spectral lines of
AGNs. They will thus have an effect on the measurements of the black hole mass
and the geometry of the AGN. This atlas of spectral simulations can serve as a
guide to future reverberation campaigns
