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Autor:
Ze-Yin Dong, Xian-Yong Bai, Song Feng, Yuan-Yong Deng, Zi-Hang Yu, Wen-Tong Ao, Xiao Yang, Zhi-Yong Zhang, Zhi-Wei Feng
Publikováno v:
Research in Astronomy and Astrophysics. 23:055015
A Fourier transform spectrometer (FTS) has been used to observe solar activities due to its ultra-high spectral resolution. However, the FTS in-band spectra are usually distorted and some artifacts appear in out-of-band regions due to nonlinear effec