Improved experiment method for intensity correlation imaging in laboratory

被引:4
作者
Beijing Institute of Tracking and Telecommunication Technology, Beijing [1 ]
100094, China
不详 [2 ]
130033, China
机构
[1] Beijing Institute of Tracking and Telecommunication Technology, Beijing
[2] Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun
来源
Guangxue Jingmi Gongcheng | / 1卷 / 83-92期
关键词
Intensity correlation imaging; Phase retrieval; Pseudothermal light; Spatial frequency spectrum; Synthetic aperture imaging;
D O I
10.3788/OPE.20152301.0083
中图分类号
学科分类号
摘要
An improved experiment method in a laboratory for intensity correlation imaging was designed to simplify the experiment processing of the intensity correlation imaging and to obtain measured data close to the actual observation. Firstly, the theory of intensity correlation imaging and its influencing factors on imaging quality were analyzed. Then, the existing intensity correlation imaging method and its disadvantages were discussed. A new experiment of intensity correlation imaging was designed and implemented by using a pseudothermal light and a CCD array, and the theories and characteristics to simulate the intensity correlation imaging by proposed method were introduced. Finally, the data analysis and imaging experiments were performed to verify the feasibility of the method. Experimental results indicate that the proposed method measures well the spatial power spectra of the objects, and the measurement noise mainly distributes in the high frequency region. Moreover, the intensity image of the object can be reconstructed by a phase retrieval algorithm when the signal-to-noise ratio is higher than 20. It concludes that this method preferably realizes the simulation of intensity correlation imaging. In the experiment, the adjustment of the intensity random fluctuation and the parameter of observing baseline are more convenient, so that the object with a small angular diameter is easy to be imaged. ©, 2015, Chinese Academy of Sciences. All right reserved.
引用
收藏
页码:83 / 92
页数:9
相关论文
共 19 条
  • [1] Wessels R.L., Vaughan R.G., Patrick M.R., Et al., High-resolution satellite and airborne thermal infrared imaging of precursory unrest and 2009 eruption at Redoubt Volcano, Alaska, Journal of Volcanology and Geothermal Research, 259, pp. 248-269, (2013)
  • [2] Deng J., Zhang W., Long F.N., Optical design of large aperture segmented mirror system, Opt. Precision Eng., 16, 1, pp. 29-34, (2008)
  • [3] Quirrenbach A., Optical interferometry, Annual Review of Astronomy and Astrophysics, 39, 1, pp. 353-401, (2001)
  • [4] Yu S.H., Wang J.L., Dong L., Et al., Field experiment data processing of Fourier telescopy based on phase spectrum analysis, Opt. Precision Eng., 20, 10, pp. 2275-2282, (2012)
  • [5] Dong L., Liu X.Y., Wang J.L., Realization of Fourier telescope technology in laboratory, Opt. Precision Eng., 16, 6, pp. 999-1002, (2008)
  • [6] Dravins D., Lebohec S., Jensen H., Et al., Optical intensity interferometry with the Cherenkov telescope array, Astroparticle Physics, 43, pp. 331-347, (2013)
  • [7] Strekalov D.V., Erkmen B.I., Yu N., Intensity interferometry for observation of dark objects, Physical Review A, 88, 5, (2013)
  • [8] Hanbury B.R., Davis J., Allen L.R., The angular diameters of 32 stars, Monthly Notices of the Royal Astronomical Society, 167, pp. 121-136, (1974)
  • [9] Hussein I.I., Scheeres D.J., Hyland D.C., Interferometric observatories in earth orbit, Journal of Guidance, Control, and Dynamics, 27, 2, pp. 297-300, (2004)
  • [10] Nunez P.D., Holmes R., Kieda D., Et al., High angular resolution imaging with stellar intensity interferometry using air Cherenkov telescope arrays, Monthly Notices of the Royal Astronomical Society, 419, 1, pp. 172-183, (2012)