Reptile Lamp Database

Spectrum 435: SUN Edit
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Full Spectrum

2010-05-23; 14:10 (solar altitude 56.6)
maple tree shade

Measurement

Brand other
other
Lamp Product Sun
Direct sunlight
Lamp ID SUN (01/2000)
Spectrometer USB2000+ (2)
Ballast - no ballast or default/unknown ballast -
Reflector
Distance 0 cm
Age 0 hours
Originator (measurement) Frances Baines
Database entry created: Sarina Wunderlich 12/Jan/2012 ; updated: Sarina Wunderlich 12/Jan/2012

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 ( 0.26 ; 0.27 ) ( 0.29 ; 0.38 ) ( 0.16 ; 0.24 ; 0.32 )
CCT 15000 Kelvin 8000 Kelvin 9500 Kelvin
distance 0.045 0.048
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) 3070 µW/cm² = 30.7 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) 3060 µW/cm² = 30.6 W/m²
UVB (EU) ( 280 nm - 315 nm) 12.9 µW/cm² = 0.129 W/m²
UVB (US) ( 280 nm - 320 nm) 24.6 µW/cm² = 0.246 W/m²
UVA+B ( 280 nm - 380 nm) 302 µW/cm² = 3.02 W/m²
Solar UVB ( 290 nm - 315 nm) 12.9 µW/cm² = 0.129 W/m²
UVA D3 regulating ( 315 nm - 335 nm) 72.9 µW/cm² = 0.729 W/m²
UVA (EU) ( 315 nm - 380 nm) 289 µW/cm² = 2.89 W/m²
UVA2 (medical definition) ( 320 nm - 340 nm) 84.1 µW/cm² = 0.841 W/m²
UVA (US) ( 320 nm - 380 nm) 277 µW/cm² = 2.77 W/m²
UVA1 (variant) ( 335 nm - 380 nm) 216 µW/cm² = 2.16 W/m²
UVA1 (medical) ( 340 nm - 400 nm) 281 µW/cm² = 2.81 W/m²
vis. UVA ( 350 nm - 380 nm) 148 µW/cm² = 1.48 W/m²
VIS Rep3 ( 350 nm - 600 nm) 1170 µW/cm² = 11.7 W/m²
VIS Rep4 ( 350 nm - 700 nm) 1340 µW/cm² = 13.4 W/m²
purple ( 380 nm - 420 nm) 224 µW/cm² = 2.24 W/m²
VIS ( 380 nm - 780 nm) 1770 µW/cm² = 17.7 W/m²
VIS2 ( 400 nm - 680 nm) 1080 µW/cm² = 10.8 W/m²
PAR ( 400 nm - 700 nm) 1100 µW/cm² = 11 W/m²
tmp ( 400 nm - 1100 nm) 2680 µW/cm² = 26.8 W/m²
blue ( 420 nm - 490 nm) 402 µW/cm² = 4.02 W/m²
green ( 490 nm - 575 nm) 329 µW/cm² = 3.29 W/m²
yellow ( 575 nm - 585 nm) 28.9 µW/cm² = 0.289 W/m²
orange ( 585 nm - 650 nm) 141 µW/cm² = 1.41 W/m²
red ( 650 nm - 780 nm) 642 µW/cm² = 6.42 W/m²
IRA ( 700 nm - 1400 nm) 1580 µW/cm² = 15.8 W/m²
IR2 ( 720 nm - 1100 nm) 1520 µW/cm² = 15.2 W/m²
IRB ( 1400 nm - 3000 nm) 0 µW/cm² = 0 W/m²
Actionspectra
Erythema 0.696 UV-Index
Pyrimidine dimerization of DNA 8.78 µW/cm²
Photoceratitis 1.01 µW/cm²
Photoconjunctivitis 0.0153 µW/cm²
DNA Damage 0.0509
Vitamin D3 2.79 µW/cm²
Photosynthesis 821 µW/cm²
Luminosity 2620 lx
Human L-Cone 378 µW/cm²
Human M-Cone 355 µW/cm²
Human S-Cone 342 µW/cm²
CIE X 341 µW/cm²
CIE Y 361 µW/cm²
CIE Z 618 µW/cm²
PAR 5060000 mol photons
Extinction preD3 25.8 e-3*m²/mol
Extinction Tachysterol 95.4 e-3*m²/mol
Exctincition PreD3 13500 m²/mol
Extinction Lumisterol 2.13 m²/mol
Exctincition Tachysterol 159000 m²/mol
Extinction 7DHC 1.64 m²/mol
L-Cone 299 µW/cm²
M-Cone 453 µW/cm²
S-Cone 601 µW/cm²
U-Cone 512 µW/cm²
UVR - ICNIRP 2004 0.462 Rel Biol Eff
Melatonin Supression 487 µW/cm²
Blue Light Hazard 404 µW/cm² (154 µW/cm² per 1000 lx)
CIE 174:2006 PreVit D3 3.04 µW/cm²
Lumen Reptil 3910 "pseudo-lx"
Vitamin D3 Degradation 5.08 µW/cm²
Actinic UV 0.462 µW/cm² (1.76 mW/klm)
Exctincition Lumisterol 3640 m²/mol
Exctincition 7DHC 2260 m²/mol
Exctincition Toxisterols 3110 m²/mol
Broadbandmeters
Solarmeter 6.2 (UVB, pre 2010) 34.5 µW/cm²
Solarmeter 6.5 (UV-Index, pre 2010) 0.86
Leybold UVB 22.9 µW/cm²
Leybold UVA 204 µW/cm²
Leybold UVC 0.000752 µW/cm²
DeltaOhm UVB 79.9 µW/cm²
DeltaOhm UVC 8.14 µW/cm²
Vernier UVB 5.94 µW/cm²
Vernier UVA 166 µW/cm²
Gröbel UVA 237 µW/cm²
Gröbel UVB 10.2 µW/cm²
Gröbel UVC -0.00706 µW/cm²
Luxmeter 2750 lx
Solarmeter 6.4 (D3) 2.69 IU/min
UVX-31 91.7 µW/cm²
IL UVB 0.0161 µW/cm²
IL UVA 237 µW/cm²
Solarmeter 6.5 (UVI, post 2010) 0.745 UV-Index
Solarmeter 6.2 (UVB, post 2010) 25.4 µW/cm² (Solarmeter Ratio = 34.1)
Solarmeter AlGaN 6.5 UVI sensor 11.3 UV Index
GenUV 7.1 UV-Index 0.732 UV-Index
Solarmeter 10.0 (Global Power) (manuf.) 38.2 W/m²
Solarmeter 4.0 (UVA) 3.64 mW/cm²
LS122 (manuf.) 1.82 W/m²
ISM400 (first guess) 39.9 W/m²
LS122 (assumption) 2.44 W/m²
ISM400_new 41.9 W/m²
Solarmeter 10.0 (Global Power) (assumption) 37.4 W/m²