text: referring to fig1 a scene 10 has a light source 12 emitting illuminating light 14 onto a surface 16 . the light striking the surface has a spectral power distribution e ( λ ) which defines the relative intensity of light at a plurality of wavelengths in the visible spectrum . in this embodiment , the light source 12 is daylight having a spectral power distribution as indicated in fig2 . alternatively the light source may be a candle , tungsten light , black body radiator , other artificial or natural light source , or a combination of any of these . referring back to fig1 illuminating light 14 strikes a point x on the surface 16 . the surface , at point x , reflects the illuminating light to produce reflected light 18 . the illuminating light 14 is not necessarily constant over the entire scene , therefore each point in the scene can receive illuminating light having a different spectral power distribution . the surface 16 is assumed to be opaque and matt and therefore the reflected light 18 at point x can be described in terms of a fraction of the illuminating light impinging upon point x . the surface does not reflect all wavelengths of light 14 in the same proportions and therefore individual fractional values representing the ratio of illuminating light 14 to reflected light 18 must be specified for each wavelength of light impinging upon the surface . the collection of all of the individual fractional values specifies the surface spectral reflectance s ( λ ) of the surface at point x . each point on the surface may have a different spectral reflectance . in this example , the surface 16 is a river valley with meadows . the spectral reflectance of this surface has been previously measured and is described by krinov in technical translation tt439 of the national research council of canada 1947 incorporated herein by reference . the spectral reflectance of this surface is repeated here in fig3 . referring back to fig1 the reflected light 18 from point x is received by a spectrometer 20 . the spectrometer performs a bandlimited spectral analysis of the reflected light 18 to produce a spectral power distribution im ( λ ) as shown in fig4 . the spectrometer represents the spectral power distribution im ( λ ) of reflected light as a plurality of light intensity samples taken at l wavelengths . this is shown at task 208 in fig7 a . referring back to fig1 the samples are communicated to a computer 22 by signal wires 24 such as found in a serial communication link . task 206 of fig7 a represents the receipt of these communicated samples . as will become apparent below , the number of light intensity samples must be at least as many as the sum of the number of basis functions used to approximate the illuminating light component plus the number of basis functions used to approximate the surface spectral reflectance component . the computer 22 in this example is a sun - 2 workstation running a 4 . 2bsd unix operating system . an applications program shown in broken outline at 26 , for performing a separation algorithm 28 is written in the c programming language and runs in conjunction with the unix operating system . the computer 22 acts to provide first programmable means . the computer 22 , operating system and applications program 26 cooperate to implement the separation algorithm 28 . alternatively , the computer 22 and software may be replaced by a hardwired electronic circuit or an analog computer . referring to fig1 a and 7b the applications program 26 includes a library 30 of illuminant basis functions and a library 32 of reflectance basis functions . the library 30 includes a plurality of illuminant basis functions eb i ( λ ) which are used in weighted proportions to represent an approximation to the spectral power distribution of the illuminating light 14 emitted by the light source 12 . this approximation is represented as a weighted sum of the illuminant basis functions according to the equation : ## equ3 ## where : ea ( λ ) is an approximation to the spectral power distribution of the illuminating light ε i is a weighting coefficient for the ith basis function , eb i ( λ ) is the ith basis function for representing illuminating light , the above equation allows the illuminating light to be characterized by an illumination vector of weights : the illuminant basis functions eb i ( λ ) in this embodiment are given by judd , deane b ., macadam , david l . and wyszecki , gunter in an article entitled &# 34 ; spectral distribution of typical daylight as a function of correlated colour temperature &# 34 ; appearing in the journal of the optical society america 54 ( 8 ): 1031 - 1040 , august 1964 , incorporated herein by reference . alternatively , the illuminant basis functions eb i ( λ ) may be fourier basis functions . the library 32 of reflectance basis functions includes a plurality of reflectance basis functions sbj ( λ ) which can be used in weighted proportions to represent an approximation to the surface spectral reflectance of a point on the surface such as point x . this approximation is represented as a weighted sum of reflectance basis functions according to the equation : ## equ4 ## where : sa ( λ ) is an approximation to the surface spectral reflectance of a point on the surface , sb j ( λ ) is the jth basis function for representing the surface spectral reflectance , the above equation allows the spectral reflectance to be characterized by a surface reflectance vector of weights : the reflectance basis functions sbj ( λ ) in this embodiment are given by cohen , j ., in dependency of the spectral reflectance curves of the munsell color chips , psychon . sci . 1 : 369 - 370 , 1964 , incorporated herein by reference . alternatively , the spectral reflectance basis functions sbj ( λ ) may be fourier basis functions . the two approximations ea ( λ ) and sa ( λ ) are multiplied together to arrive at an approximation ia ( λ ) to the spectral power distribution of the reflected light according to the equation : the equation produces a set of product pairs eb i ( λ ) sb j ( λ ) which must be linearly independent . at task 214 in fig7 a , the program 26 acts to generate a weighting coeffecient ε i for each of m illuminant basis functions eb i ( λ ) for describing the illuminating light 14 . the use of m illuminant basis functions requires that the program generate m respective illuminant weighting coefficients . thus , the illumination vector of weights ε =( ε 1 , ε 2 , ε 3 , . . . ε m ) has m components . the number m of basis functions required to describe the illuminating light 14 depends upon the desired accuracy of the approximation ea ( λ ). statistical analysis of illumination measurements provides as many basis functions as desired . an adequate approximation ea ( λ ) is obtained using four or five illuminant basis functions . the judd reference listed above provides up to five ( i . e . m = 5 ) illuminant basis functions which have been found to provide reasonable approximations to the illuminating light in most outdoor scenes . at task 212 , the program 26 also acts to generate a weighting coefficient σ j for each of n reflectance basis functions sbj ( λ ) for describing the reflectance of a point on the surface 16 . the use of n reflectance basis functions requires that the program generate n respective surface reflectance weighting coeffecients . thus , the surface reflectance vector of weights σ =(∝ 1 , σ 2 , σ 3 , . . . σ n ) has n components . statistical analysis of surface reflectance measurements provides as many basis functions as desired . an adequate approximation sa ( λ ) is obtained using four to seven reflectance basis functions . the cohen reference above provides up to four ( n = 4 ) reflectance basis functions which have been found to provide reasonable approximations to the surface reflectance of many surfaces . the program 26 generates the illumination vector of weights ε and the surface reflectance vector of weights σ according to equations ( 1 ) and ( 2 ) below , the equations being derived using the calculus of variations : ## equ6 ## referring to fig7 a and 7b to begin solving the equations for ε and σ , task 210 of the program 26 generates a first illumination vector of weights assuming the illluminating light is of a standard type such as daylight at noon . at task 212 , this first illumination vector of weights is then used in equation 1 to solve for a first surface reflectance vector of weights . this can be accomplished by standard methods since equation 1 is linear in σj . upon obtaining values for the first surface reflectance vector of weights , at task 214 , these values are then used in equation 2 to obtain a second illumination vector of weights . this second illumination vector is then used in equation 1 to produce a second surface reflectance vector . this second surface reflectance vector is then used in equation 2 to produce a third illumination vector and so on . the alternate solving of equations 1 and 2 is an iterative process which is carried out until the generated illumination vectors converge and the generated surface reflectance vectors also converge . the value to which the illumination vector converges defines the resultant illumination vector and the value to which the surface reflectance vector converges defines the resultant surface reflectance vector of point x on the surface 16 . the effect of the above two equations is to employ the least squares method to derive an appropriate illumination vector and an appropriate surface reflectance vector such that the approximation ia ( λ ) is fitted closely to within acceptable limits of the measured im ( λ ). in effect , the illumination vector and the surface reflectance vector are selected such that the following mathematical relation is a minimum : ## equ7 ## as exemplified in tasks 216 and 218 , the illumination vector and the surface reflectance vector are iteratively recalculated until the approximation ia ( λ ) is such that the above expression is a minimum . the illumination vector components and the reflectance vector components which make the above equation take on its minimum value are the illumination and surface reflectance vectors which best define the illuminating light 14 and the surface reflectance of the point x on the surface 16 . upon generating the resultant illumination vector ε and the resultant surface reflectance vector σ , the approximation to the illuminating light ea ( λ ) and the approximation to the surface spectral reflectance sa ( λ ) are produced with task 220 and 222 according to the equations : ## equ8 ## where : ea ( λ ) is an approximation to the spectral power distribution of the illuminating light ε i is a weighting coefficient for the ith basis function , the weighting coefficient being from the generated illumination vector of weights , eb i ( λ ) is the ith basis function for representing illuminating light . m is the number of illuminant basis functions used . ## equ9 ## where : sa ( λ ) is an approximation to the surface spectral reflectance of a point on the surface , σj is a weighting coefficient for the jth basis function , the weighting coefficient being from the generated illumination vector of weights , sbj ( λ ) is the jth basis function for representing the surface spectral reflectance , the program represents the illuminating light approximation ea ( λ ) as a plurality of light intensity samples taken at a plurality of wavelengths . similarly , the program represents the surface reflectance approximation as a plurality of reflectance samples taken at a plurality of wavelengths . the samples are represented as electrical signals on wires 42 and 44 as exemplified by task 224 . the signals are supplied to an interface 34 for a video display terminal 36 as shown in fig1 . alternatively the electrical signals may be supplied to an interface ( not shown ) for transmission over a communications channel , or for providing a general connection point to wires 42 and 44 . alternatively , the signals may be used in further processing steps performed by the computer . for instance , the reflectance samples for the scene may be processed by the computer using conventional techniques of color science to compute committee internationale d &# 39 ; eclairage ( cie ) color tri - stimulus coordinates . these coordinates may be used to provide signals for accurately displaying the scene on a wide variety of color display media , printing devices or systems . the apparatus may also be used to develop signals for implementing a color filter . in this application , the illumination constituent is found at a few selected points in the scene and interpolation methods are used to find the illumination constituent at points therebetween . consequently , the illumination constituent need not necessarily be calculated at each point in the scene and therefore computation time can be reduced . using this approach , the illumination constituent need only be repeatedly used in the first iterative process equation to find the surface reflectance vector and hence the surface relectance at each point in the scene . upon determining the surface reflectance constituent at each point . correction signals for implementing the color filter may be produced using conventional techniques . referring to fig5 a plurality of reflectance samples are displayed in graphical form . the actual surface reflectance of the surface is indicated by the solid line 38 . the approximation to the surface reflectance obtained through the use of the iterative process described earlier is indicated by the broken line 40 . referring to fig6 a second embodiment of the invention is shown . in general , the second embodiment replaces the spectrometer of the first embodiment with a plurality of y sensors for receiving light reflected by the illuminated surface and includes an illumination approximation algorithm 133 incorporated into an applications program 126 . the scene and elements of the second embodiment are similar to corresponding items of the first embodiment . items of the second embodiment which correspond to items of the first embodiment are indicated by the addition of 100 to numerical references of the first embodiment . the reflected light 118 from point x is received by sensors , in this case by first , second and third sensors 119 , 121 and 123 respectively . each sensor has a respective spectral sensitivity and produces a respective sensor signal ρy responsive to the intensity and the spectral content of the light received at the sensor . the spectral sensitivity of any individual sensor is specified by the relation : ry ( λ ) is the spectral sensitivity of the yth sensor as a function of λ ; and i ( λ ) is the intensity of the light reflected by the illuminated surface as a function of λ . in this embodiment the spectral sensitivity , r y ( λ ), for each sensor is illustrated as item 302 in fig8 . in this example , the sensors have respective broadband spectral sensitivities corresponding generally to the colours red , green and blue . the sensors provide first , second and third electrical sensor signals 125 , 127 , 129 representing scalar numerical values corresponding to the intensity of the colours red , green and blue respectively in the reflected light 118 . the first , second and third electrical sensor signals 125 , 127 and 129 are supplied to a computer 122 programmed with the applications program 126 as illustrated by 306 in fig8 . the applications program is similar to program 26 described in the first embodiment except that in addition to a separation algorithm 128 and basis function libraries 130 and 132 , the program includes an illumination approximation algorithm 133 . under the illumination approximation algorithm the program 126 processes the sensor signals 125 , 127 , 129 to produce data signals on wires 124 , the signals representing a measured spectral power distribution im ( λ ) of the reflected light 118 . the program acts to generate a fourier weighting coefficient α y for each of y fourier basis functions fb y ( λ ) 304 for describing an approximation iam ( λ ) to the measured spectral power distribution im ( λ ) of the reflected light 118 according to the relation : ## equ10 ## the fourier coefficients are generated by using the above relation to generate approximations to the numerical values produced by each of the sensors , the approximations being generated by the relation : task 308 illustrates that each sensor approximation ρ ay is then compared to the actual values produced by the sensors , and the squares of the differences between each approximation and actual sensor values are summed to produce an error value according to the relation : er =[( ρ . sub . 1 - ρ . sub . a1 ). sup . 2 +( ρ . sub . 2 - ρ . sub . a2 ). sup . 2 +( ρ . sub . 3 - ρ . sub . a3 ) . sup . 2 . . . ( ρ . sub . y - ρ . sub . ay ). sup . 2 ] numerical methods are used to choose fourier coefficients such that the error in the above relation is set to a minimum . in task 310 , the fourier coefficients which satisfy these criteria are then used in conjunction with the fourier basis functions fb y ( λ ) according to the relation : ## equ12 ## the data signals 124 represent iam ( λ ) as a plurality of light intensity samples taken at l wavelengths . at task 312 , the signals are passed to the separation algorithm 128 and are interpreted as im ( λ ) samples such as supplied by the spectrometer described in the first embodiment . the iam ( λ ) samples are then used by the separation algorithm to determine the illumination signals and the reflectance signals as described in connection with the first embodiment . these signals appear on wires 142 and 144 respectively . the signals may then be used with an interface 134 and a video display terminal 136 as described in connection with the first embodiment . while specific embodiments of the invention have been described , such embodiments should be considered illustrative of the invention only and not as limiting the scope of the invention as construed in accordance with the accompanying claims .