[1] Uitenbroek H, Noyes R W, Rabin D. Imaing spectroscopy of the solar CO lines at 4.67 microns[J]. Astrophysical Journal, 1994,432(1):L67-L70.
[2] Livingston W, Solanki S, Muglach K, et al. The beat of the solar chromosphere's cold heart[J]. Astronomy and Astrophysics, 1996,315:303-311.
[3] Hall D N B, Noyes R W, Ayres T R. The identification of 13C16O in the infrared sunspot spectrum and the determination of the solar 12C13C abundance ratio[J]. Astrophysical Journal, 1972,171:615-617.
[4] Penn M J, Schad T, Cox E. probing the solar atmosphere using oscillations of infrared CO spectral lines[J]. Astrophysical Journal, 2011,734(1):47-56.
[5] 尤建圻,王传晋,陆静,等. 太阳HeI 10830光谱单色扫描装置[J]. 天文学报, 1993,34(4):374-379. You J Q, Wang C J, Lu J, et al. An equipment for solar two dimension spectra observation in HeI 10830[J]. Acta Astronomica Sinica, 1993,34(4):374-379.
[6] Fang C, Chen P F, Li Z, et al. A new multi-wavelength solar telescope:OPTICAL and near-infrared solar eruption tracer (ONSET)[J]. Research in Astronomy & Astrophysics, 2013,13(12):1509-1517.
[7] 许方宇,徐稚,徐世春,等. 抚仙湖一米新真空太阳望远镜6米近红外光谱仪装调及太阳1.56微米光谱的初步观测结果[J]. 天文研究与技术, 2014,11(2):168-175. Xu F Y, Xu Z, Xu S C, et al. Installation/adjustment of a 6m near-infrared spectrograph for the 1m new vacuum solar telescope in the fuxian-lake solar-observation station and preliminary observation results of solar spectra around 1.56μm using the spectrograph[J]. Astronomical Research and Technology, 2014,11(2):168-175.
[8] 冯志伟,杨潇,白先勇,等. 用于天文成像探测的IRFPA性能参数测试[J]. 影像科学与光化学, 2017,35(2):140-146. Feng Z W, Yang X, Bai X Y, et al. Performance parameter test of IRFPA used in astronomy imaging detection[J]. Imaging Science an Photochemistry, 2017,35(2):140-146.
[9] Pierre L, Daniel R, Francois L, et al. Observational Astrophysics[M]. 3rd Edition. London:Springer, 2012. 509-595. |