Blue Lamp, 100W, 20cm
Spectrum 658: TG-PR-BDE-100-001 Edit
DeleteMeasurement
| Brand |
Pro Rep UK Brand - associated with Peregrine Livefoods (wholesaler) |
|---|---|
| Lamp Product |
Pro Rep Blue Dusk Effect 100W Blue Lamp, 100W |
| Lamp ID |
TG-PR-BDE-100-001 (07/2022) Blue lamp from Pro Rep, 100W |
| Spectrometer | FLAME UV-Vis (E) |
| Ballast | - no ballast or default/unknown ballast - |
| Reflector | |
| Distance | 20 cm |
| Age | 5 hours |
| Originator (measurement) | Thomas Griffiths |
Database entry created:
Thomas Griffiths (Tomaskas Ltd.)
4/Feb/2023 ; updated:
Thomas Griffiths (Tomaskas Ltd.)
4/Feb/2023
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 | ( 0.25 ; 0.23 ) | ( 0.31 ; 0.47 ) | ( 0.17 ; 0.26 ; 0.39 ) |
| CCT | 130000 Kelvin | 6900 Kelvin | 8600 Kelvin |
| distance | 0.13 | 0.12 | |
| 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) 4310 µW/cm² = 43.1 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) 4110 µW/cm² = 41.1 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) 9.45 µW/cm² = 0.0945 W/m² Solar UVB ( 290 nm - 315 nm) 0 µW/cm² = 0 W/m² UVA D3 regulating ( 315 nm - 335 nm) 0 µW/cm² = 0 W/m² UVA (EU) ( 315 nm - 380 nm) 9.45 µW/cm² = 0.0945 W/m² UVA2 (medical definition) ( 320 nm - 340 nm) 0 µW/cm² = 0 W/m² UVA (US) ( 320 nm - 380 nm) 9.45 µW/cm² = 0.0945 W/m² UVA1 (variant) ( 335 nm - 380 nm) 9.45 µW/cm² = 0.0945 W/m² UVA1 (medical) ( 340 nm - 400 nm) 19.9 µW/cm² = 0.199 W/m² vis. UVA ( 350 nm - 380 nm) 7.83 µW/cm² = 0.0783 W/m² VIS Rep3 ( 350 nm - 600 nm) 159 µW/cm² = 1.59 W/m² VIS Rep4 ( 350 nm - 700 nm) 245 µW/cm² = 2.45 W/m² purple ( 380 nm - 420 nm) 25.8 µW/cm² = 0.258 W/m² VIS ( 380 nm - 780 nm) 1570 µW/cm² = 15.7 W/m² VIS2 ( 400 nm - 680 nm) 171 µW/cm² = 1.71 W/m² PAR ( 400 nm - 700 nm) 227 µW/cm² = 2.27 W/m² tmp ( 400 nm - 1100 nm) 4290 µW/cm² = 42.9 W/m² blue ( 420 nm - 490 nm) 74.6 µW/cm² = 0.746 W/m² green ( 490 nm - 575 nm) 44.2 µW/cm² = 0.442 W/m² yellow ( 575 nm - 585 nm) 3.71 µW/cm² = 0.0371 W/m² orange ( 585 nm - 650 nm) 17.3 µW/cm² = 0.173 W/m² red ( 650 nm - 780 nm) 1400 µW/cm² = 14 W/m² IRA ( 700 nm - 1400 nm) 4060 µW/cm² = 40.6 W/m² IR2 ( 720 nm - 1100 nm) 3870 µW/cm² = 38.7 W/m² IRB ( 1400 nm - 3000 nm) 0 µW/cm² = 0 W/m²
Actionspectra
Erythema 0.00246 UV-Index Pyrimidine dimerization of DNA 0.00294 µW/cm² Photoceratitis 0 µW/cm² Photoconjunctivitis 0 µW/cm² DNA Damage 7.12E-6 Vitamin D3 0 µW/cm² Photosynthesis 232 µW/cm² Luminosity 364 lx Human L-Cone 52.6 µW/cm² Human M-Cone 48.7 µW/cm² Human S-Cone 60.7 µW/cm² CIE X 53.9 µW/cm² CIE Y 49.6 µW/cm² CIE Z 112 µW/cm² PAR 1100000 mol photons Extinction preD3 0 e-3*m²/mol Extinction Tachysterol 0 e-3*m²/mol Exctincition PreD3 19.6 m²/mol Extinction Lumisterol 0 m²/mol Exctincition Tachysterol 340 m²/mol Extinction 7DHC 0 m²/mol L-Cone 44.7 µW/cm² M-Cone 68.6 µW/cm² S-Cone 103 µW/cm² U-Cone 48.7 µW/cm² UVR - ICNIRP 2004 0.00167 Rel Biol Eff Melatonin Supression 82.4 µW/cm² Blue Light Hazard 69.1 µW/cm² (190 µW/cm² per 1000 lx) CIE 174:2006 PreVit D3 0 µW/cm² Lumen Reptil 572 "pseudo-lx" Vitamin D3 Degradation 0 µW/cm² Actinic UV 0.00167 µW/cm² (0.0459 mW/klm) Exctincition Lumisterol 0 m²/mol Exctincition 7DHC 0 m²/mol Exctincition Toxisterols 15.5 m²/mol
Broadbandmeters
Solarmeter 6.2 (UVB, pre 2010) 0.0732 µW/cm² Solarmeter 6.5 (UV-Index, pre 2010) 0.000817 Leybold UVB 0 µW/cm² Leybold UVA 7.92 µW/cm² Leybold UVC 0 µW/cm² DeltaOhm UVB 0.174 µW/cm² DeltaOhm UVC 0 µW/cm² Vernier UVB 0 µW/cm² Vernier UVA 3.7 µW/cm² Gröbel UVA 7.72 µW/cm² Gröbel UVB 0.014 µW/cm² Gröbel UVC 0 µW/cm² Luxmeter 372 lx Solarmeter 6.4 (D3) 0.00255 IU/min UVX-31 0.624 µW/cm² IL UVB 5.34E-5 µW/cm² IL UVA 9.42 µW/cm² Solarmeter 6.5 (UVI, post 2010) 0.000347 UV-Index Solarmeter 6.2 (UVB, post 2010) 0.00304 µW/cm² (Solarmeter Ratio = 8.75) Solarmeter AlGaN 6.5 UVI sensor 0.00342 UV Index GenUV 7.1 UV-Index 0.00333 UV-Index Solarmeter 10.0 (Global Power) (manuf.) 70.3 W/m² Solarmeter 4.0 (UVA) 0.196 mW/cm² LS122 (manuf.) 5.7 W/m² ISM400 (first guess) 88.5 W/m² LS122 (assumption) 6.24 W/m² ISM400_new 98.2 W/m² Solarmeter 10.0 (Global Power) (assumption) 72.3 W/m²