Fluorescent Excitation from White LEDs

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Fluorescent Excitation from White LEDs David R. Wyble Munsell Color Science Laboratory Chester F. Carlson Center for Imaging Science Rochester Institute of Technology

The Problem? original images from Wikimedia and NASA

The Problem content <400nm 1%? 1% 0% 9% percent of 300-800nm content between 300-400nm original images from Wikimedia and NASA

Motivation Growth of solid state lighting for indoor illumination applications is inevitable Many benefits over conventional illumination Cost Life Energy usage Environmental concerns Some issues: Color rendering Fluorescence

Characterizing Fluorescence Bispectral spectrophotometry moving slit selects excitation wavelength light source excitation monochromator Record complete emitted spectrum for each excitation wavelength Any detected light not of the same wavelength as excitation indicates fluorescence Example shows material emitting green and red light when being excited by green sample spectral detector emission monochromator

Characterizing Fluorescence Excitation wavelength (μ) 380 390 770 780 Emission wavelength (λ) 380 β R 380 390 β R 390 : 760 770 β R 770 780 β R 780 Donaldson Matrix Here: Excitation wavelength (μ) is 300-780nm. Emission wavelength (λ) is measured from 380-780nm

Characterizing Fluorescence Excitation wavelength (μ) 380 390 770 780 Emission wavelength (λ) 380 β R 380 390 β R 390 : 760 770 β R 770 780 β R 780 Donaldson Matrix Here: Excitation wavelength (μ) is 300-780nm. Emission wavelength (λ) is measured from 380-780nm

Fluorescence calculations Reflected Radiance Factor β R,λ [the corrected diagonal] Donaldson matrix Reflected TSV s Fluorescent Radiance Factor Fluorescent TSV s β F,µ,λ W R = k β F,λ = W F = k λ µ λ β R,λ s λ w λ Δλ s µ β F,µ,λ s λ β F,λ s λ w λ Δλ λ = emission µ = excitation W R = X,Y,Z w λ = x λ, y λ, z λ Total TSV s W T = W R + W F Calculate CIELAB from these tristimulus values using D65, 1931 observer.

Paper Radiance Factors 1.2 1 radiance factor 0.8 0.6 0.4 Reflected Luminescent Total 0.2 0 380 430 480 530 580 630 680 730 780 wavelength (nm) Illuminant D65 Epson 1047049

The Experiment Set of 6 typical white office papers Donaldson matrix Bispectral measurements Process Colorimetric data Normalized source data White LED

The Experiment Set of 6 typical white office papers Donaldson matrix Bispectral measurements Process Colorimetric data Normalized source data White LED

Light Source Details White LEDs Blue LED + yellow phosphor RGB 405 nm LED + yellow phosphor Source normalization 1931 2 Y tristimulus value = 100 Best compromise for the intended application

LEDs with Peak at 405 radiance 300 350 400 450 500 550 600 650 700 750

Synthetic LEDs Synthetic 405+Y radiance Original B+Y 300 350 400 450 500 550 600 650 700 750 Maintain the shape of the yellow emission.

Normalized Virtual Sources CIE D65 Cool white CIE A normalized units 300 350 400 450 500 550 600 650 700 750 wavelength (nm)

Normalized LED Output normalized units 405 3 NVLAP-1 SSL-5 RGB2 SSL-3 300 350 400 450 500 550 600 650 700 750 wavelength (nm)

The Experiment Set of 6 typical white office papers Donaldson matrix Bispectral measurements Process Colorimetric data Normalized source data White LED

Substrate Details White office paper Standard Epson stock All exhibit fluorescence to some degree 1.2 1 radiance factor 0.8 0.6 0.4 Reflected Luminescent Total Illuminant D65 Epson 1047049 0.2 0 380 430 480 530 580 630 680 730 780 wavelength (nm)

Substrate Details radiance 1047049 Q5462A S041062 S041160 S04124 S041341 300 350 400 450 Excitation spectra

What Do We Expect? radiance 300 350 400 450 500 excitation range sources

Results 1.2 1 radiance factor 0.8 0.6 0.4 Reflected Total 0.2 0 380 430 480 530 580 630 680 730 780 wavelength (nm) Calculate a color difference between the reflected and total radiance factors. How visible is the change imposed by the luminescent radiance factor?

Results 1.2 1 radiance factor 0.8 0.6 0.4 Reflected Total 0.2 0 380 430 480 530 580 630 680 730 780 wavelength (nm) Calculate a color difference between the reflected and total radiance factors. How visible is the change imposed by the luminescent radiance factor?

Results Light Sources papers RGB2 405 3 NVLAP-1 SSL-5 SSL-3 CIE D65 CIE A Cool white 1047049 4.20 12.61 0.11 0.91 4.58 9.25 5.50 1.95 Q5462A 0.68 7.35 0.02 0.20 0.74 3.25 2.04 0.74 S041062 5.24 13.39 0.06 1.09 5.72 10.48 6.14 2.24 S04124 7.06 19.64 0.02 1.52 7.69 14.12 8.45 3.16 S041160 7.93 21.28 0.01 1.70 8.64 15.31 9.19 3.49 S041341 5.61 14.97 0.04 1.19 6.11 11.70 6.94 2.49 ΔE * ab between luminescent and total radiance factors.

Results ΔE * ab 25 20 15 sources illuminants 1047049 Q5462A S041062 S04124 S041160 S041341 papers 10 5 0 RGB2 405 3 NVLAP-1 SSL-5 SSL-3 D65 A Cool white Interpretation: this shows the color difference that would be expected by illuminating each paper under the given light source if paper OBAs were removed. Put another way, this is as though two papers were viewed side by side, one with and one without fluorescent OBAs.

Results ΔE * ab 25 20 15 sources illuminants 1047049 Q5462A S041062 S04124 S041160 S041341 papers 10 5 0 RGB2 405 3 NVLAP-1 SSL-5 SSL-3 D65 A Cool white Interpretation: this shows the color difference that would be expected by illuminating each paper under the given light source if paper OBAs were removed. Put another way, this is as though two papers were viewed side by side, one with and one without fluorescent OBAs.

0.1 0.075 0.05 0.025 0 excitation 300 325 350 375 400 radiance 300 350 400 450 500 wavelength (nm)

Conclusions and Recommendations Commercially available white LEDs (RGB, B+Y) do not adequately excite office paper optical brightening agents. An LED configuration including a lower wavelength source, such as the 405nm blue, can provide the necessary excitation to preserve paper appearance. Alternative strategies could include adjusting the paper OBA chemistry. None of the issues are show stoppers compared to the other significant benefits of solid state lighting. Printing, packaging and other graphic arts applications could potentially require process adjustments.

Future Work Add substrates and sources Your contributions are encouraged Data or samples Simulation images Consider other aspects of sources CRI, cost, lifetime, etc Luminescence - safety markings Not future work (for this researcher): Engineer a new LED Adjust OBA chemistry

Acknowledgments Funding for this work came in part from Munsell Color Science Laboratory RIT s Center for Imaging Science X-rite Incorporated Many thanks for technical discussions and the sharing of data from: Dr Cameron Miller (NIST) Dr Art Springsteen (Avian Technologies) Mr Jim Leland (Gamma Scientific)