determination of the albedo and the *g*-factor in both the FUV (1350-1750 [Å]{}) and NUV (1750-2850 [Å]{}) bands [@suj09; @suj10]. Most of these studies showed that the interstellar grain causes a strong forward scattering in the FUV, with a moderate albedo, which is in good agreement with theoretical predictions.

The Orion-Eridanus Superbubble (henceforth OES) is a large hot bubble with a diameter of $\sim$30$^\circ$ across the sky located in the Orion and Eridanus constellations. Its distance is known to be $\sim$155 pc to the near-side and $\sim$586 pc to the far-side of the bubble, and its near edge is considered to interact with the expanding shell of the Local Bubble [@bur96]. The OES has been observed extensively in various wavelengths, ranging from X-ray to radio. Enhanced soft X-ray emission seen at its inner cavities is the evidence of the hot gas (T $\sim$ 10$^6$ K) occupying its inner parts [@hei99]. Two prominent filamentary H$\alpha$ shells, known as arcs A and B, have been observed at the boundaries of these hot cavities [@rey98; @bou01]. The presence of 21 cm radiation of neutral hydrogen (T $\sim$ 10$^{2-3}$ K) was also noted outside the hot bubble (Brown et al. 1995). The dust extinction 