Reptile Lamp Database

Spectrum 487: McKinlay9 Edit
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Full Spectrum

Measurement

Brand other
other
Lamp Product Tungsten Halogen 9
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 9
Lamp ID McKinlay9 (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 ( 0.44 ; 0.4 ) ( 0.58 ; 0.29 ) ( 0.5 ; 0.29 ; 0.15 )
CCT 3000 Kelvin 3000 Kelvin 3000 Kelvin
distance 0.0027 0.0037
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) 9290 µW/cm² = 92.9 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) 2270 µW/cm² = 22.7 W/m²
UVB (EU) ( 280 nm - 315 nm) 1.67 µW/cm² = 0.0167 W/m²
UVB (US) ( 280 nm - 320 nm) 2.05 µW/cm² = 0.0205 W/m²
UVA+B ( 280 nm - 380 nm) 18.1 µW/cm² = 0.181 W/m²
Solar UVB ( 290 nm - 315 nm) 1.67 µW/cm² = 0.0167 W/m²
UVA D3 regulating ( 315 nm - 335 nm) 2.92 µW/cm² = 0.0292 W/m²
UVA (EU) ( 315 nm - 380 nm) 16.5 µW/cm² = 0.165 W/m²
UVA2 (medical definition) ( 320 nm - 340 nm) 3.26 µW/cm² = 0.0326 W/m²
UVA (US) ( 320 nm - 380 nm) 16.1 µW/cm² = 0.161 W/m²
UVA1 (variant) ( 335 nm - 380 nm) 13.5 µW/cm² = 0.135 W/m²
UVA1 (medical) ( 340 nm - 400 nm) 23.3 µW/cm² = 0.233 W/m²
vis. UVA ( 350 nm - 380 nm) 10.5 µW/cm² = 0.105 W/m²
VIS Rep3 ( 350 nm - 600 nm) 475 µW/cm² = 4.75 W/m²
VIS Rep4 ( 350 nm - 700 nm) 1000 µW/cm² = 10 W/m²
purple ( 380 nm - 420 nm) 24.3 µW/cm² = 0.243 W/m²
VIS ( 380 nm - 780 nm) 1540 µW/cm² = 15.4 W/m²
PAR ( 400 nm - 700 nm) 979 µW/cm² = 9.79 W/m²
blue ( 420 nm - 490 nm) 93.9 µW/cm² = 0.939 W/m²
green ( 490 nm - 575 nm) 249 µW/cm² = 2.49 W/m²
yellow ( 575 nm - 585 nm) 26.1 µW/cm² = 0.261 W/m²
orange ( 585 nm - 650 nm) 320 µW/cm² = 3.2 W/m²
red ( 650 nm - 780 nm) 824 µW/cm² = 8.24 W/m²
IRA ( 700 nm - 1400 nm) 5400 µW/cm² = 54 W/m²
IRB ( 1400 nm - 3000 nm) 2880 µW/cm² = 28.8 W/m²
Actionspectra
Erythema 0.133 UV-Index
Pyrimidine dimerization of DNA 1.15 µW/cm²
Photoceratitis 0.189 µW/cm²
Photoconjunctivitis 0.00308 µW/cm²
DNA Damage 0.0117
Vitamin D3 0.625 µW/cm²
Photosynthesis 698 µW/cm²
Luminosity 2610 lx
Human L-Cone 409 µW/cm²
Human M-Cone 287 µW/cm²
Human S-Cone 74.6 µW/cm²
CIE X 394 µW/cm²
CIE Y 363 µW/cm²
CIE Z 144 µW/cm²
PAR 4890000 mol photons
Extinction preD3 2.81 e-3*m²/mol
Extinction Tachysterol 9.5 e-3*m²/mol
Exctincition PreD3 1340 m²/mol
Extinction Lumisterol 0.577 m²/mol
Exctincition Tachysterol 13500 m²/mol
Extinction 7DHC 0.384 m²/mol
L-Cone 382 µW/cm²
M-Cone 218 µW/cm²
S-Cone 111 µW/cm²
U-Cone 48.7 µW/cm²
UVR - ICNIRP 2004 0.11 Rel Biol Eff
Melatonin Supression 130 µW/cm²
Blue Light Hazard 84.5 µW/cm² (32.4 µW/cm² per 1000 lx)
CIE 174:2006 PreVit D3 0.703 µW/cm²
Lumen Reptil 2000 "pseudo-lx"
Vitamin D3 Degradation 0.45 µW/cm²
Actinic UV 0.112 µW/cm² (0.43 mW/klm)
Exctincition Lumisterol 790 m²/mol
Exctincition 7DHC 521 m²/mol
Exctincition Toxisterols 205 m²/mol
Broadbandmeters
Solarmeter 6.2 (UVB, pre 2010) 2.53 µW/cm²
Solarmeter 6.5 (UV-Index, pre 2010) 0.178
Leybold UVB 1.89 µW/cm²
Leybold UVA 12 µW/cm²
Leybold UVC 0 µW/cm²
DeltaOhm UVB 3.92 µW/cm²
DeltaOhm UVC 0.433 µW/cm²
Vernier UVB 1.05 µW/cm²
Vernier UVA 8.01 µW/cm²
Gröbel UVA 13.2 µW/cm²
Gröbel UVB 1.16 µW/cm²
Gröbel UVC 0.000161 µW/cm²
Solarmeter 6.4 (D3) 0.557 IU/min
UVX-31 4.75 µW/cm²
IL UVB 0.00117 µW/cm²
IL UVA 14.2 µW/cm²
Solarmeter 6.5 (UVI, post 2010) 0.142 UV-Index
Solarmeter 6.2 (UVB, post 2010) 1.54 µW/cm² (Solarmeter Ratio = 10.9)
Solarmeter AlGaN 6.5 UVI sensor 1.39 UV Index
GenUV 7.1 UV-Index 0.0738 UV-Index
Solarmeter 10.0 (Global Power) 61.1 W/m²
Solarmeter 4.0 (UVA) 0.253 mW/cm²
LS122 57.7 W/m²
ISM400 73.3 W/m²