Reptile Lamp Database

Spectrum 488: McKinlay10 Edit
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Full Spectrum

Measurement

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.

Spectrum in the visible wavelength range

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, 338451, 511513 ), 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.

Spectrum in the vitamin D3 active wavelength range

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
then any Solarmeter 6.2 reading multiplied with 0.7 (0.7=13.8/19.6) is an estimate of UVB irradiance for this specific lamp. If you do so, always make sure, that the calculated (effective) irradiance is valid. The calculated value is not valid, if the lamp's spectrum is not measured in the relevant range.

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
PAR ( 400 nm - 700 nm) 2740 µW/cm² = 27.4 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
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
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) 149 W/m²
Solarmeter 4.0 (UVA) 0.788 mW/cm²
LS122 115 W/m²
ISM400 176 W/m²