  Emission in forbidden lines of oxygen, neon, and other species are commonly
used to trace winds from protoplanetary disks. Using Cloudy, we calculate such
emission for parametrized wind models of the magnetothermal type, following Bai
et al. (2016). These models share characteristics with both photoevaporative
and magnetocentrifugal winds, which can be regarded as end members, and are
favored by recent theoretical research. Both broad and narrow low-velocity
components of the lines can be produced with plausible wind parameters,
something that traditional wind models have difficulty with. Line luminosities,
blueshifts, and widths, as well as trends of these with accretion luminosity
and disk inclination, are in general accord with observations
