Computer Simulation for the Observation of the 1.56μm Fe Ⅰ Spectral Line of Solar Magnetic Field

It makes an interesting idea and work to use the IRFPA made in China and the solar spectrometer at Yunnan Observatory to probe into the local magnetic field on solar surface by the observation of NIR Fe I line at 1.56μm. The computer simulation is presented in this paper. The influence of the apparatus effects and noises in the observation results are also discussed in detail.