[1] |
BORN M E. Wolf principles of optics[J]. Pergamon Press, 1980, 6:188-189.
|
[2] |
ROUSSET G, MUGNIER L M, CASSAING F, et al. Imaging with multi-aperture optical telescopes and an application[J]. Comptes Rendus de l'Acad mie des Sciences-Series IV-Physics, 2001, 2(1):17-25. http://www.ingentaconnect.com/content/els/12962147/2001/00000002/00000001/art01158
|
[3] |
MERMELSTEIN M. Optical synthetic aperture array:US, 6548820 B1[P]. 2003-04-15.
|
[4] |
CASSAING F, SORRENTE B, FLEURY B, et al.. Optical design of a Michelson wide-field multiple-aperture telescope[J]. SPIE, 2004, 5249:220-229. doi: 10.1117/12.515215
|
[5] |
KNIGHT J S, LIGHTSEY P, BARTO A. Predicted JWST imaging performance[J]. SPIE, 2012, 8442:84422G. https://www.researchgate.net/publication/258718427_Predicted_JWST_imaging_performance
|
[6] |
CHANAN G, OHARA C, TROY M. Phasing the mirror segments of the Keck telescopes Ⅱ:the narrow-band phasing algorithm[J]. Applied Optics, 2000, 39(25):4706-4714. doi: 10.1364/AO.39.004706
|
[7] |
CHANAN G, TROY M, DEKENS F, et al.. Phasing the mirror segments of the Keck telescopes:the broadband phasing algorithm[J]. Applied Optics, 1998, 37(1):140-155. doi: 10.1364/AO.37.000140
|
[8] |
MACINTOSH B, TROY M, DOYON R, et al.. Extreme adaptive optics for the Thirty Meter Telescope[J]. SPIE, 2006, 6272:62720N-15. http://adsabs.harvard.edu/abs/2006SPIE.6272E..0NM
|
[9] |
BROWN A M, ARMSTRONG T, CHADWICK P M, et al.. Flasher and muon-based calibration of the GCT telescopes proposed for the cherenkov telescope array[J]. Research in Astronomy & Astrophysics, 2015, 15(8):1095-1124. http://www.oalib.com/paper/3708931
|
[10] |
HORNSCHEMEIER A E, BRANDT W N, GARMIRE G P, et al.. The Chandra Deep Survey of the Hubble Deep Field-North Area[J]. The Astrophysical J., 2001, 554(2):742. doi: 10.1086/apj.2001.554.issue-2
|
[11] |
BUCKLEY D A H, BARNES S I, BURGH E B, et al.. Commissioning of the Southern African Large Telescopes (SALT) first-generation instruments[J]. SPIE, 2008, 7014:701407-15. https://www.researchgate.net/profile/Andrew_Sheinis/publication/252818340_Commissioning_of_the_Southern_African_Large_Telescope_(SALT)_First-Generation_Instruments/links/54eba5a20cf2082851be4d06.pdf?inViewer=true&pdfJsDownload=true&disableCoverPage=true&origin=publication_detail
|
[12] |
GILMOZZI R, SPYROMILIO J. The european extremely large telescope (E-ELT)[J]. The Messenger, 2007, 127(11):3. https://www.eso.org/sci/publications/messenger/archive/no.127-mar07/messenger-no127-11-19.pdf
|
[13] |
DIERICKX P, GILMOZZI R. Progress of the OWL 100-m telescope conceptual design[C]. Astronomical Telescopes and Instrumentation. International Society for Optics and Photonics, Munich, Germany, 2000:290-299.
|
[14] |
LENZEN R, BRANDL B, BRANDNER W. The science case for exoplanets and star formation using mid-IR instrumentation at the OWL telescope[C]. The Scientific Requirements for Extremely Large Telescopes, 2005, 1(232):329-333.
|
[15] |
LAJOIE C P, SOUMMER R, PUEYO L, et al.. Planning and developing JWST CORONAGRAPHS OPerations[J]. Iau General Assembly, 2015:22. http://adsabs.harvard.edu/abs/2015IAUGA..2257743L
|
[16] |
JOHNS M, ANGEL J R P, SHECTMAN S, et al.. Status of the giant magellan telescope (GMT) project[J]. SPIE, 2004, 5489:441-453. https://www.researchgate.net/publication/247647325_Status_of_the_Giant_Magellan_Telescope_GMT_Project?_sg=7CMQlENRA73-BdrPKQFckugloqXHmXqJ3vhWjEBe_5wv9lbMZx988Fa1nv2epKvczOYXVqo-IA4YraEwYm7Uug
|
[17] |
RUTTEN R J, HAMMERSCHLAG R H, BETTONVIL F C M, et al.. DOT tomography of the solar atmosphere-I. Telescope summary and program definition[J]. Astronomy & Astrophysics, 2004, 413(3):1183-1189. http://citeseerx.ist.psu.edu/viewdoc/bookmark?doi=10.1.1.494.1692&site=connotea
|
[18] |
朱仁璋, 丛云天, 王鸿芳, 等.全球高分光学量概述(二):欧洲[J].航天器工程, 2016, 25(1):95-118. http://www.cnki.com.cn/Article/CJFDTOTAL-HTGC201601015.htm
|
[19] |
BECKERS J M, ULICH B L, WILLIAMS J T. Performance of The Multiple Mirror Telescope (MMT) I. MMT-the first of the advanced technology telescopes[C]. 1982 Astronomy Conferences. International Society for Optics and Photonics, Muich, Germany, 1982:2-8.
|
[20] |
HILL J M, ASHBY D S, BRYNNEL J G, et al.. The large binocular telescope:binocular all the time[J]. SPIE, 2014, 9145:914502.
|
[21] |
BONANOS A Z, STANEK K A. Reanalysis of very large telescope data for M83 with image subtraction-nicefold increase in number of cepheids[J]. Astrophysical J., 2003, 591(2):L111-L114 doi: 10.1086/377073
|
[22] |
CHUNG S J, MILLER D W, WECK O L D. ARGOS testbed:study of multidisciplinary challenges of future spaceborne interferometric arrays[J]. Optical Engineering, 2004, 43(43):2156-2167. https://www.researchgate.net/publication/268571251_Multidisciplinary_Control_of_a_Sparse_Interferometric_Array_Satellite_Testbed
|
[23] |
PITMAN J T, DUNCAN A, STUBBS D, et al. Remote sensing space science enabled by the multiple instrument distributed aperture sensor (MIDAS) concept[J]. SPIE, 2004, 5555:301-310. https://www.researchgate.net/publication/260077353_Remote_sensing_space_science_enabled_by_the_Multiple_Instrument_Distributed_Aperture_Sensor_MIDAS_concept
|
[24] |
FRINK S, QUIRRENBACH A, FISCHER D, et al.. A strategy for identifying the grid stars for the Space Interferometry Mission (SIM)[J]. Publications of the Astronomical Society of the Pacific, 2001, 113(780):173-187. doi: 10.1086/pasp.2001.113.issue-780
|
[25] |
KALTENEGGER L, FRIDLUND M. Characteristics of proposed 3 and 4 telescope configurations for Darwin and TPF-I[J]. Proceedings of the International Astronomical Union, 2005, 1(C200):255-258. doi: 10.1017/S1743921306009410
|
[26] |
HILL J M. The large binocular telescope[J]. Applied Optics, 2010, 49(16):D115-D122. doi: 10.1364/AO.49.00D115
|
[27] |
TRAUB W A. Combining beams from separated telescopes[J]. Applied Optics, 1986, 25(4):528-532. doi: 10.1364/AO.25.000528
|
[28] |
MATHER J, STOCKMAN H S, GREENBEL T. Next generation space telescope[J]. SPIE, 2000, 4013:2~16 http://www.nasa.gov/news/budget/image_jwst.html
|
[29] |
LEVOY M, CHEN B, VAISH V, et al.. Synthetic aperture confocal imaging[J]. Acm Transactions on Graphics, 2004, 23(3):825-834. doi: 10.1145/1015706
|
[30] |
ZHAO Y. Large sky area multi-object fiber spectroscopic telescope[J]. Bulletin of the Chinese Academy of Sciences, 2011(3):231-232. http://www.docin.com/p-1544731231.html
|
[31] |
ZHOU Z, WANG D, WANG Y. Effect of noise on the performance of image restoration in an optical sparse aperture system[J]. J. Optics, 2011, 13(7):075502. doi: 10.1088/2040-8978/13/7/075502
|
[32] |
魏小峰, 耿则勋, 宋向.光学合成孔径复原图像的振铃探测与消除[J].光学精密工程, 2014, 22(11):3091-3099. http://www.cnki.com.cn/Article/CJFDTOTAL-GXJM201411029.htmWEI X F, GENG Z X, SONG X. Detection and removal of ringing artifact for optical synthetic aperture restoration image[J]. Optics & Precision Engineering, 2014, 22(11):3091-3099.(in Chinese) http://www.cnki.com.cn/Article/CJFDTOTAL-GXJM201411029.htm
|
[33] |
刘政, 王胜千, 饶长辉.一种基于远场图像的稀疏光学合成孔径系统共相探测新方法的仿真研究[J].物理学报, 2012, 61(3):0390501. http://www.cnki.com.cn/Article/CJFDTOTAL-WLXB201203082.htmLIU ZH, WANG SH Q, RAO CH H, et al.. Analysis of an Co-phasing detecting method based on far-field images of sparse-optical-synthetic-aperture system[J]. Acta Physica Sinica, 2012, 61(3):0390501.(in Chinese) http://www.cnki.com.cn/Article/CJFDTOTAL-WLXB201203082.htm
|
[34] |
中国科学院光电技术研究所.光电所在分离镜面光学合成孔径关键技术研究上取得重要进展[EB/OL].[2016-03-29].
|