  We treat transformation properties of external radiation fields in the proper
frame of a plasma moving with constant speed. The specific spectral energy
densities of external isotropic and accretion-disk radiation fields are derived
in the comoving frame of relativistic outflows, such as those thought to be
found near black-hole jet and gamma-ray burst sources. Nonthermal electrons and
positrons Compton-scatter this radiation field, and high-energy protons and
ions interact with this field through photomeson and photopair production. We
revisit the problem of the Compton-scattered spectrum associated with an
external accretion-disk radiation field, and clarify a past treatment by the
authors. Simple expressions for energy-loss rates and Thomson-scattered spectra
are given for ambient soft photon fields consisting either of a surrounding
external isotropic monochromatic radiation field, or of an azimuthally
symmetric, geometrically thin accretion-disk radiation field. A model for
blazar emission is presented that displays a characteristic spectral and
variability behavior due to the presence of a direct accretion-disk component.
The disk component and distinct flaring behavior can be bright enough to be
detected from flat spectrum radio quasars with {\it GLAST}. Spectral states of
blazars are characterized by the relative importance of the accretion-disk and
scattered radiation fields and, in the extended jet, by the accretion disk,
inner jet, and cosmic microwave background radiation fields.
