We have developed a Monte Carlo code, which solves the problem of radiative transfer in anisotropically scattering atmosphere. The radiative code is flexible in handlings of the system geometry, the distribution of scattering particles, and the source-particle geometry. This code treats the case of highly forward throwing scattering. As performance tests, we have compared the result of Monte Carlo calculations with that of Quasi-Diffusion method for a spherically symmetric cloud model.

• 박찬(서울대학교 천문학과) | PARK CHAN (Department of Astronomy, Seoul National University)
• 홍승수(서울대학교 천문학과) | HONG SEUNG SOO (Department of Astronomy, Seoul National University)