[1] Heacox W D. On the application of optical-fiber image scramblers to astronomical spectroscopy[J]. The Astronomical Journal, 1986, 92(1): 219-229.
[2] Heacox W D. Radial image transfer by cylindrical, step-index optical waveguides[J]. J Opt Soc Am A, 1987, 4(3): 488-493.
[3] Boisse I, Bouchy F, Chazelas B, et al. Consequences of spectrograph illumination for the accuracy of radial-velocimetry[C]. European Physical Journal Conferences, 2011, 16(2): 309-315.
[4] Barnes S I, MacQueen P J. A high-efficiency fibre double-scrambler prototype[C]. SPIE, 2010, 7735: 773567.
[5] Avila G, Singh P. Optical fiber scrambling and light pipes for high accuracy radial velocities measurements[C]. SPIE, 2008, 7018: 70184W.
[6] Feger T, Brucalassi A, Grupp F, et al. A test bed for simultaneous measurement of fiber near and far-field for the evaluation of fiber scrambling properties[C]. SPIE, 2012, 8446: 844692.
[7] Casse M, Vieira F. Comparison of the scrambling properties of bare optical fibers with microlens coupled fibers[C]. SPIE, 1997, 2871: 1187-1196.
[8] Steinmetz T, Wilken T, Araujo-Hauck C, et al. Laser frequency combs for astronomical observations[J]. Science, 2008, 321(5894): 1335-1337.
[9] Murphy M T, Udem T, Holzwarth R, et al. High-precision wavelength calibration of astronomical spectrographs with laser frequency combs[J]. Monthly Notices of the Royal Astronomical Society, 2007, 380(2): 839-847.
[10] Wilken T, Lovis C, Manescau A, et al. High-precision calibration of spectrographs[J]. Monthly Notices of the Royal Astronomical Society, 2010, 405(1): L16-L20.
[11] Wilken T, Curto G L, Probst R A, et al. A spectrograph for exoplanet observations calibrated at the centimetre-per-second level[J]. Nature, 2012, 485(7400): 611-614.
[12] Han Hainian, Wei Zhiyi, Zhao Gang. Astro-frequency-combs and high precision measurement of the radial velocity of celestial bodies[J]. Physics, 2012, 41(4): 249-255.
[13] Jiang Mingda, Xiao Dong, Zhu Yongtian, The progress in high precision astronomical radial velocity technique[J] Progress in Astronomy, 2012, 30(2): 264-253.
[14] Bouchy F, Connes P. Autoguider locked on a fiber input for precision stellar radial velocities[J]. Astronomy & Astrophysics Supplement Series, 1999, 136(1): 193-204.
[15] Yang Cong, Han Jian, Wu Yuanjie, et al. Theoretical and experimental study on suppression of speckle from a multimode optical fiber by dynamic scrambling[J]. Laser & Optoelctronics Progress, 2015, 52(9): 090602.
[16] Yan L S, Yao X S, Lin L, et al. Improved beam uniformity in multimode fibers using piezoelectric-based spatial mode scrambling for medical applications[J]. Optical Engineering, 2008, 47(9): 090502.
[17] Halverson S, Roy A, Mahadevan S, et al. An efficient, compact, and versatile fiber double scrambler for high precision radial velocity instruments[J]. The Astrophysical Journal, 2015, 806(1): 61-69.
[18] Allington-Smith J, Murray G, Lemke U. Simulation of complex phenomena in optical fibres[J]. Monthly Notices of the Royal Astronomical Society, 2012, 427(2): 919-933.
[19] Allington-Smith J, Dunlop G. Lemke U. et al. End effects in optical fibres[J]. Monthly Notices of the Royal Astronomical Society, 2013, 436(4): 3492-3499.
[21] Chi Zeying, Chen Wenjian, Li Wusen. Fiber optics, theories and application[M]. 2nd ed. Beijing: Publishing House of Electronics Industry, 2014: 16-31.
[22] Han Jian, Xiao Dong. Near and far field scrambling properties of polygonal core optical fiber[J], Acta Optica Sinica, 2016, 36(4): 0406003.