研究成果藝廊 > 天文物理理論與觀測整合研究計畫(CHARMS)
研究成果藝廊
天文物理理論與觀測整合研究計畫(CHARMS)
Polarization Calculation and Visualization from MHD Simulation Data |
圖片來源: Väisälä, Shang, Krasnopolsky et al.
A sample picture based on the radiative transfer code Perspective exploring a very early stage disk formed within the MHD model of Li et al. (2014). The picture shows gas column density and linear polarization component q along the line of sight, inclined 15 degrees from the midplane. The early disk in the model shows a spiral-like shape, presumably created by the magnetic field aligned along the rotational plane of the original cloud. (Väisälä, Shang et al., a work in progress)
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