Spectrum 488: McKinlay10 Edit
DeleteMeasurement
| Brand |
other other |
|---|---|
| Lamp Product |
Tungsten Halogen 10 MacKinlay, A. F., Whillock, J., & Meulemans, C. C. E. (1989). Ultraviolet radiation and blue-light emissions from spotlights incorporating tungsten halogen lamps. National Radiological Protection Board. Lamp 10 |
| Lamp ID |
McKinlay10 (11/2013) |
| Spectrometer | - |
| Ballast | - no ballast or default/unknown ballast - |
| Reflector | |
| Distance | 30 cm |
| Age | 20 hours |
| Originator (measurement) | Publication |
Database entry created:
Sarina Wunderlich
2/Nov/2013 ; updated:
Sarina Wunderlich
2/Nov/2013
Colorimetry
Colorimetry is the science to describe physically the human color perception. The wavelength range 380 nm - 780 nm is visible to humans and detected by three different photoreceptors. Many Reptiles see the range 350 nm - 800 nm and have an additional UV photoreceptor in their retina.
Whereas a spectrometer measures the intensity in every tiny wavelength interval resulting in thousands of individual intensities, the human eye only measures three intensities detected by the three cones. The same is true for the reptile eye with usually three or four photoreceptors. Effectively the detailled spectrum displayed above reduces to a much compacter bar graph displayed below. The photoreceptor sensitivites from these L-Cone, M-Cone, S-Cone, and U-Cone are used, they are chosen as an average of measured reptile photoreceptor sensitivity curves. The bar graph also shows as reference the intensity seen by the three or four photoreceptors for average sunlight (id 1).
From these three numbers the colour coordinate and the correlated colour temperature for humans are calculated using the CIE standard method. I adapted this concept to a "3 cone reptile (M,S,U)" and a "4 cone reptile (L,M,S,U)". I am sure, that this adaption to other colour spaces makes sense mathematically and this is also done in scientific research regarding colour vision of animals, however I have not seen calculation of colour temperatures for other animals in the scientific literature. Even if it is hypothetical, at least this shows, how arbitrary the colour temperature is, and that the colour temperature calculated for humans does not apply to reptiles. The colour spaces also show the colour coordinates of different phases of daylight ((ids 1, 338 – 451, 511 – 513 ), indicated by crosses, coloured in the appriximate colour perceived by a human.
| Human (CIE) | 3 cone reptile | 4 cone reptile | |
|---|---|---|---|
| Cone Excitation | |||
| Colour Coordinate | ( 0.42 ; 0.4 ) | ( 0.56 ; 0.3 ) | ( 0.48 ; 0.29 ; 0.16 ) |
| CCT | 3200 Kelvin | 3100 Kelvin | 3200 Kelvin |
| distance | 0.00087 | 0.0044 | |
| colour space | 3-D-graph not implemented yet |
Vitamin D3 Analysis
Vitamin D3 is produced by UVB radiation around 300 nm. 7DHC/ProD3 present in the skin is converted to PreD3 when absorbing an UV photon. PreD3 can be converted back to ProD3, to Lumisterol, or to Tachysterol when absorbing another UV photon or can be converted to Vitamin D3 in a warm environment.
This process prevents any overdose of vitamin D3 from UV radiation with a spectrum similar to sunlight. As a comparison the solar spectra at 20°(id:14) and at 85°(id:21) solar angle are shown.
The ratio of the two solarmeters 6.2 (UVB) and 6.5 (UV index) readings has proven a useful and very simply number to acess the spectral shape in the vitamin-d3-active region.
Effective Irradiances
Effective irradiances are calculated for all ranges, actionspectra and radiometers currently present in this database.
The calculation method is a numerical implementation (Simpson's rule) of the formula
To learn more about calculating effective irradiances and radiometers I recommend this excellent report on UVB meters: Characterizing the Performance of Integral Measuring UV-Meters (pdf).
The numbers in the following tables can also be used to estimate certain (effective) irradiances from radiomer readings. Example: If the database lists
- range: UVB (US) = 13.8 µW/cm²
- radiometer: Solarmeter 6.2 = 19.6 µW/cm²
Ranges
total ( 0 nm - 0 nm) 20300 µW/cm² = 203 W/m² UVC ( 0 nm - 280 nm) 0 µW/cm² = 0 W/m² non-terrestrial ( 0 nm - 290 nm) 0 µW/cm² = 0 W/m² total2 ( 250 nm - 880 nm) 5980 µW/cm² = 59.8 W/m² UVB (EU) ( 280 nm - 315 nm) 2.86 µW/cm² = 0.0286 W/m² UVB (US) ( 280 nm - 320 nm) 3.84 µW/cm² = 0.0384 W/m² UVA+B ( 280 nm - 380 nm) 52.5 µW/cm² = 0.525 W/m² Solar UVB ( 290 nm - 315 nm) 2.86 µW/cm² = 0.0286 W/m² UVA D3 regulating ( 315 nm - 335 nm) 8.07 µW/cm² = 0.0807 W/m² UVA (EU) ( 315 nm - 380 nm) 49.6 µW/cm² = 0.496 W/m² UVA2 (medical definition) ( 320 nm - 340 nm) 9.06 µW/cm² = 0.0906 W/m² UVA (US) ( 320 nm - 380 nm) 48.7 µW/cm² = 0.487 W/m² UVA1 (variant) ( 335 nm - 380 nm) 41.6 µW/cm² = 0.416 W/m² UVA1 (medical) ( 340 nm - 400 nm) 74.3 µW/cm² = 0.743 W/m² vis. UVA ( 350 nm - 380 nm) 32.8 µW/cm² = 0.328 W/m² VIS Rep3 ( 350 nm - 600 nm) 1420 µW/cm² = 14.2 W/m² VIS Rep4 ( 350 nm - 700 nm) 2810 µW/cm² = 28.1 W/m² purple ( 380 nm - 420 nm) 82.4 µW/cm² = 0.824 W/m² VIS ( 380 nm - 780 nm) 4160 µW/cm² = 41.6 W/m² VIS2 ( 400 nm - 680 nm) 2420 µW/cm² = 24.2 W/m² PAR ( 400 nm - 700 nm) 2740 µW/cm² = 27.4 W/m² tmp ( 400 nm - 1100 nm) 10000 µW/cm² = 100 W/m² blue ( 420 nm - 490 nm) 296 µW/cm² = 2.96 W/m² green ( 490 nm - 575 nm) 738 µW/cm² = 7.38 W/m² yellow ( 575 nm - 585 nm) 74.1 µW/cm² = 0.741 W/m² orange ( 585 nm - 650 nm) 864 µW/cm² = 8.64 W/m² red ( 650 nm - 780 nm) 2100 µW/cm² = 21 W/m² IRA ( 700 nm - 1400 nm) 11900 µW/cm² = 119 W/m² IR2 ( 720 nm - 1100 nm) 6950 µW/cm² = 69.5 W/m² IRB ( 1400 nm - 3000 nm) 5550 µW/cm² = 55.5 W/m²
Actionspectra
Erythema 0.18 UV-Index Pyrimidine dimerization of DNA 1.73 µW/cm² Photoceratitis 0.243 µW/cm² Photoconjunctivitis 0.0035 µW/cm² DNA Damage 0.0137 Vitamin D3 0.798 µW/cm² Photosynthesis 1940 µW/cm² Luminosity 7480 lx Human L-Cone 1160 µW/cm² Human M-Cone 836 µW/cm² Human S-Cone 237 µW/cm² CIE X 1100 µW/cm² CIE Y 1040 µW/cm² CIE Z 455 µW/cm² PAR 13600000 mol photons Extinction preD3 4.54 e-3*m²/mol Extinction Tachysterol 15.9 e-3*m²/mol Exctincition PreD3 2250 m²/mol Extinction Lumisterol 0.665 m²/mol Exctincition Tachysterol 24400 m²/mol Extinction 7DHC 0.438 m²/mol L-Cone 1070 µW/cm² M-Cone 659 µW/cm² S-Cone 358 µW/cm² U-Cone 160 µW/cm² UVR - ICNIRP 2004 0.139 Rel Biol Eff Melatonin Supression 407 µW/cm² Blue Light Hazard 269 µW/cm² (36 µW/cm² per 1000 lx) CIE 174:2006 PreVit D3 0.873 µW/cm² Lumen Reptil 5850 "pseudo-lx" Vitamin D3 Degradation 0.787 µW/cm² Actinic UV 0.141 µW/cm² (0.189 mW/klm) Exctincition Lumisterol 995 m²/mol Exctincition 7DHC 617 m²/mol Exctincition Toxisterols 426 m²/mol
Broadbandmeters
Solarmeter 6.2 (UVB, pre 2010) 5.01 µW/cm² Solarmeter 6.5 (UV-Index, pre 2010) 0.233 Leybold UVB 3.48 µW/cm² Leybold UVA 36.4 µW/cm² Leybold UVC 0 µW/cm² DeltaOhm UVB 9.41 µW/cm² DeltaOhm UVC 0.9 µW/cm² Vernier UVB 1.47 µW/cm² Vernier UVA 23 µW/cm² Gröbel UVA 39.4 µW/cm² Gröbel UVB 1.87 µW/cm² Gröbel UVC -0.00032 µW/cm² Luxmeter 7230 lx Solarmeter 6.4 (D3) 0.728 IU/min UVX-31 11.5 µW/cm² IL UVB 0.00232 µW/cm² IL UVA 43.2 µW/cm² Solarmeter 6.5 (UVI, post 2010) 0.189 UV-Index Solarmeter 6.2 (UVB, post 2010) 3.27 µW/cm² (Solarmeter Ratio = 17.3) Solarmeter AlGaN 6.5 UVI sensor 2.18 UV Index GenUV 7.1 UV-Index 0.13 UV-Index Solarmeter 10.0 (Global Power) (manuf.) 149 W/m² Solarmeter 4.0 (UVA) 0.788 mW/cm² LS122 (manuf.) 177 W/m² ISM400 (first guess) 176 W/m² LS122 (assumption) 163 W/m² ISM400_new 207 W/m² Solarmeter 10.0 (Global Power) (assumption) 152 W/m²