[1] A.Wootten.The Atacama Large Millimeter Array (ALMA) [C].SPIE,2003,4837:110-118
[2] J.Payne,B.Shillue,A.Vaccari.Photonic techniques for use on the atacama large millimeter array [C].Proc.IEEE MWP,1999.105-108
[3] J.Payne,B.Shillue.Photonic techniques for local oscillator generation and distribution in millimeter-wave radio astronimy [C].Proc.IEEE MWP,2002.9-12
[4] Pengbo Shen,Phillip A.Davies,W.P.Shillue et al..Millimetre wave generation using an optical comb generator with optical phase-locked loops [C].Proc.IEEE MWP,2002.101-104
[8] Bill Shillue.High-frequency local oscillator transmission for the atacama large millimeter array (ALMA) [C].Digest of the LEOS Summer Topical Meetings (IEEE),2005.119-120
[9] B.Shillue,S.AlBanna,L.D′Addario.Transmission of low phase noise,low phase drift millimeter-wavelength references by a stabilized fiber distribution system [C].IEEE MWP,2004.201-204
[10] B.Shillue.ALMA LO Distribution Round Trip Phase Correction.ALMA Memo JHJ443,http://www.alma.nrao.edu/memos/html-memos/alma443/memo443.pdf
[11] K.Sato,T.Hara,S.Kuji et al..Development of an ultrastable fiber optic frequency distribution system using an optical delay control module [J].IEEE Trans.Instrumentation and Measurment,2000,49(1):19-24
[12] M.Calhoun,R.Sydnor,W.Diener.A stabilized 100-Megahertz and 1-gigahertz reference frequency distribution for cassini radio science [C].The Interplanetary Network Progress Report,2002.42-148
[13] Longsheng Ma.Delivering the same optical frequency at two places:accurate cancellation of phase noise introduced by an optical fiber or other time-varying path [J].Opt.Lett.,1994,19(21):1777-1779
[14] L.D′Addario,M.Stennes.Transmission of timing references to sub-picosecond precision over optical fiber [C].SPIE,1998,3357:691-701
[15] L.A.Ferreira,J.L.Santos,F.Farahi.Polarization-induced noise in a fiber-optic Michelson interferometer with Faraday rotator mirror elements [J].Appl.Opt.,1995,34(28):6399-6402