Taken from website, it is likely that the spectrometer is not calibrated for absolute irradiance.
Spectrum 548: SunStripII35Reptile Edit
DeleteMeasurement
| Brand |
Econlux/Terra-Solutions Econlux GmbH www.terra-solutions.de www.econlux.de |
|---|---|
| Lamp Product |
Solar Raptor SunStrip II 35 Reptile |
| Lamp ID |
SunStripII35Reptile (07/2020) generic ID |
| Spectrometer | - |
| Ballast | - no ballast or default/unknown ballast - |
| Reflector | |
| Distance | 0 cm |
| Age | 0 hours |
| Originator (measurement) | Publication |
Database entry created:
Sarina Wunderlich
7/Jul/2020 ; updated:
Sarina Wunderlich
8/Jun/2021
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 | ( 0.31 ; 0.31 ) | ( 0.44 ; 0.43 ) | ( 0.29 ; 0.31 ; 0.3 ) |
| CCT | 7100 Kelvin | 4500 Kelvin | 5000 Kelvin |
| distance | 0.091 | 0.074 | |
| 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) 1000 µW/cm² = 10 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) 1000 µW/cm² = 10 W/m² UVB (EU) ( 280 nm - 315 nm) 0 µW/cm² = 0 W/m² UVB (US) ( 280 nm - 320 nm) 0 µW/cm² = 0 W/m² UVA+B ( 280 nm - 380 nm) 13.4 µW/cm² = 0.134 W/m² Solar UVB ( 290 nm - 315 nm) 0 µW/cm² = 0 W/m² UVA D3 regulating ( 315 nm - 335 nm) 3.6 µW/cm² = 0.036 W/m² UVA (EU) ( 315 nm - 380 nm) 13.4 µW/cm² = 0.134 W/m² UVA2 (medical definition) ( 320 nm - 340 nm) 5.28 µW/cm² = 0.0528 W/m² UVA (US) ( 320 nm - 380 nm) 13.4 µW/cm² = 0.134 W/m² UVA1 (variant) ( 335 nm - 380 nm) 9.82 µW/cm² = 0.0982 W/m² UVA1 (medical) ( 340 nm - 400 nm) 53.4 µW/cm² = 0.534 W/m² vis. UVA ( 350 nm - 380 nm) 5.62 µW/cm² = 0.0562 W/m² VIS Rep3 ( 350 nm - 600 nm) 784 µW/cm² = 7.84 W/m² VIS Rep4 ( 350 nm - 700 nm) 982 µW/cm² = 9.82 W/m² purple ( 380 nm - 420 nm) 64.5 µW/cm² = 0.645 W/m² VIS ( 380 nm - 780 nm) 989 µW/cm² = 9.89 W/m² VIS2 ( 400 nm - 680 nm) 920 µW/cm² = 9.2 W/m² PAR ( 400 nm - 700 nm) 932 µW/cm² = 9.32 W/m² tmp ( 400 nm - 1100 nm) 943 µW/cm² = 9.43 W/m² blue ( 420 nm - 490 nm) 307 µW/cm² = 3.07 W/m² green ( 490 nm - 575 nm) 310 µW/cm² = 3.1 W/m² yellow ( 575 nm - 585 nm) 42.5 µW/cm² = 0.425 W/m² orange ( 585 nm - 650 nm) 203 µW/cm² = 2.03 W/m² red ( 650 nm - 780 nm) 60.7 µW/cm² = 0.607 W/m² IRA ( 700 nm - 1400 nm) 11.9 µW/cm² = 0.119 W/m² IR2 ( 720 nm - 1100 nm) 5.28 µW/cm² = 0.0528 W/m² IRB ( 1400 nm - 3000 nm) 0 µW/cm² = 0 W/m²
Actionspectra
Erythema 0.00886 UV-Index Pyrimidine dimerization of DNA 0.0891 µW/cm² Photoceratitis 0 µW/cm² Photoconjunctivitis 0 µW/cm² DNA Damage 3.9E-5 Vitamin D3 0 µW/cm² Photosynthesis 642 µW/cm² Luminosity 2860 lx Human L-Cone 424 µW/cm² Human M-Cone 363 µW/cm² Human S-Cone 245 µW/cm² CIE X 387 µW/cm² CIE Y 397 µW/cm² CIE Z 482 µW/cm² PAR 4230000 mol photons Extinction preD3 0.368 e-3*m²/mol Extinction Tachysterol 1.67 e-3*m²/mol Exctincition PreD3 315 m²/mol Extinction Lumisterol 0 m²/mol Exctincition Tachysterol 4430 m²/mol Extinction 7DHC 0 m²/mol L-Cone 354 µW/cm² M-Cone 390 µW/cm² S-Cone 377 µW/cm² U-Cone 117 µW/cm² UVR - ICNIRP 2004 0.00519 Rel Biol Eff Melatonin Supression 350 µW/cm² Blue Light Hazard 256 µW/cm² (89.6 µW/cm² per 1000 lx) CIE 174:2006 PreVit D3 0 µW/cm² Lumen Reptil 2900 "pseudo-lx" Vitamin D3 Degradation 0.0865 µW/cm² Actinic UV 0.00519 µW/cm² (0.0181 mW/klm) Exctincition Lumisterol 10.8 m²/mol Exctincition 7DHC 1.42 m²/mol Exctincition Toxisterols 116 m²/mol
Broadbandmeters
Solarmeter 6.2 (UVB, pre 2010) 0.941 µW/cm² Solarmeter 6.5 (UV-Index, pre 2010) 0.00463 Leybold UVB 0.406 µW/cm² Leybold UVA 14.2 µW/cm² Leybold UVC 0 µW/cm² DeltaOhm UVB 3.48 µW/cm² DeltaOhm UVC 0.286 µW/cm² Vernier UVB 0 µW/cm² Vernier UVA 8.54 µW/cm² Gröbel UVA 11.7 µW/cm² Gröbel UVB 0.11 µW/cm² Gröbel UVC 0 µW/cm² Luxmeter 2950 lx Solarmeter 6.4 (D3) 0.0145 IU/min UVX-31 4 µW/cm² IL UVB 0.000509 µW/cm² IL UVA 13.4 µW/cm² Solarmeter 6.5 (UVI, post 2010) 0.00411 UV-Index Solarmeter 6.2 (UVB, post 2010) 0.787 µW/cm² (Solarmeter Ratio = 191) Solarmeter AlGaN 6.5 UVI sensor 0.0346 UV Index GenUV 7.1 UV-Index 0.0132 UV-Index Solarmeter 10.0 (Global Power) (manuf.) 10 W/m² Solarmeter 4.0 (UVA) 0.456 mW/cm² LS122 (manuf.) 0 W/m² ISM400 (first guess) 6.58 W/m² LS122 (assumption) 0.323 W/m² ISM400_new 5.18 W/m² Solarmeter 10.0 (Global Power) (assumption) 9.53 W/m²