Interests in the use of thin foils as light attenuators and signal generators for energetic particle instruments in space have led to the measurement of transmittance of thin C and Si/C foils at 1216 Å, where the most intense and ubiquitous photons in the solar system reside. Our results indicate that 1) a transmittance of < 7 × 10 −4 can be achieved with 7 μg/cm 2 Si on 1.7 μg/cm 2 C; 2) Si/C composite foil with a thin carbon layer is more effective in blocking UV radiation and less likely to change its particle energy threshold under ion-irradiation than a pure carbon foil of identical areal density prior to exposure to ions; and 3) transmittance of Si/C foils of known Si and C thicknesses cannot be accurately predicted, but must be measured.