• Acta Optica Sinica
  • Vol. 42, Issue 2, 0233001 (2022)
Xiaowen Dong, Yang Xu*, Cheng Gao, and Changjun Li
Author Affiliations
  • College of Computer Science and Software Engineering, University of Science and Technology Liaoning, Anshan, Liaoning 114051, China
  • show less
    DOI: 10.3788/AOS202242.0233001 Cite this Article Set citation alerts
    Xiaowen Dong, Yang Xu, Cheng Gao, Changjun Li. Calculation of Light Source Corrected Color Temperature Based on Cone Fundamental Space[J]. Acta Optica Sinica, 2022, 42(2): 0233001 Copy Citation Text show less
    Distribution of blackbody locus and chromaticity coordinates of 401 SPDs in u-v plane
    Fig. 1. Distribution of blackbody locus and chromaticity coordinates of 401 SPDs in u-v plane
    Distribution of chromaticity coordinates of 401 SPDs in uc-vc space under different scale factors. (a) Scale factor provided by formula (9); (b) scale factor provided by formula (10); (c) scale factor provided by formula (12)
    Fig. 2. Distribution of chromaticity coordinates of 401 SPDs in uc-vc space under different scale factors. (a) Scale factor provided by formula (9); (b) scale factor provided by formula (10); (c) scale factor provided by formula (12)
    CCT mapping under different scale factors. (a) Scale factor provided by formula (9); (b) scale factor provided by formula (10); (c) scale factor provided by formula (12)
    Fig. 3. CCT mapping under different scale factors. (a) Scale factor provided by formula (9); (b) scale factor provided by formula (10); (c) scale factor provided by formula (12)
    Distribution of chromaticity coordinates of 401 SPDs in different coordinate spaces. (a) xF-yF space; (b) uF-vF space
    Fig. 4. Distribution of chromaticity coordinates of 401 SPDs in different coordinate spaces. (a) xF-yF space; (b) uF-vF space
    CCT mapping under different coordinate spaces. (a) xF-yF space; (b) uF-vF space
    Fig. 5. CCT mapping under different coordinate spaces. (a) xF-yF space; (b) uF-vF space
    Shape of spectra that produce the maximum color temperature error
    Fig. 6. Shape of spectra that produce the maximum color temperature error
    Chromaticity coordinateScale factor
    (xc,yc),(uc,vc),(u'c,v'c)Formula (9)
    (xc,yc),(uc,vc),(u'c,v'c)Formula (10)
    (xc,yc),(uc,vc),(u'c,v'c)Formula (12)
    (l,s)Formula (9)
    (xF,yF),(uF,vF),(u'F,v'F)Formula (12)
    Table 1. Chromaticity coordinates based on L, M and S under different sets of scale factors
    Chromaticity coordinate spaceScale factorMmean,1Mmedian,1Mmax,1
    xc-ycFormula (9)122268698
    Formula (10)1951102649
    Formula (12)149852060
    uc-vcFormula (9)1743617652
    Formula (10)102621387
    Formula (12)4831851
    u'c-v'cFormula (9)1753617759
    Formula (10)140792082
    Formula (12)6843936
    lc-scFormula (9)86254023
    Table 2. Summary of CCT of cone fundamental space
    Chromaticity coordinate spaceScale factorMmean,2Mmedian,2Mmax,2
    xF-yFFormula (12)158941985
    uF-vFFormula (12)4221540
    u'F-v'FFormula (12)100521553
    Table 3. Summary of CCT after cone fundamental space transformed to XYZ space
    Xiaowen Dong, Yang Xu, Cheng Gao, Changjun Li. Calculation of Light Source Corrected Color Temperature Based on Cone Fundamental Space[J]. Acta Optica Sinica, 2022, 42(2): 0233001
    Download Citation