Resulting spatially integrated X-ray DOP and flux spectra for injected beamed electron distributions with E_H = 100 keV without turbulent scattering, and with turbulent scattering (using λ_s, 0 = 2 × 10⁸ cm or λ_s, 0 = 2 × 10⁹ cm) situated in the coronal loop over a distance of [−10″, +10″] from the loop apex. Each use the following identical electron and plasma properties of: δ = 5, E_c = 20 keV (vertical grey dotted line), a beamed distribution and Ṅ = 7 × 10³⁵ e s⁻¹, and coronal plasma properties of: n = 3 × 10¹⁰ cm⁻³ and T = 20 MK, plotted for a flare located at a heliocentric angle of θ = 60°. All DOP spectra include an albedo component and a coronal thermal component (EM = 0.9 × 10⁴⁸ cm⁻³). The results suggest that a lack of coronal turbulent scattering could be detectable from the DOP spectrum.