Leftmost LED
Spectrum 635: TG-GYPR-LED-10W-7.0-002 Edit
DeleteMeasurement
| Brand |
Get Your Pet Right Australian Company - https://www.facebook.com/Get-Your-Pet-Right-1600516193502216/ |
|---|---|
| Lamp Product |
GYPR UVB LED Bar 7.0 (Unbranded) Unbranded Version of the UVB LED Bar from Get Your Pet Right |
| Lamp ID |
TG-GYPR-LED-10W-7.0-002 (12/2022) Leftmost LED of GYPR UVB LED Bar 7.0 (Unbranded) |
| Spectrometer | FLAME UV-Vis (E) |
| Ballast | - no ballast or default/unknown ballast - |
| Reflector | |
| Distance | 20 cm |
| Age | 50 hours |
| Originator (measurement) | Thomas Griffiths |
Database entry created:
Thomas Griffiths (Tomaskas Ltd.)
19/Dec/2022 ; updated:
Thomas Griffiths (Tomaskas Ltd.)
19/Dec/2022
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 ; 0.34 ) | ( 0.3 ; 0.29 ) | ( 0.23 ; 0.23 ; 0.23 ) |
| CCT | 6600 Kelvin | 8200 Kelvin | 6800 Kelvin |
| distance | 0.046 | 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.
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) 514 µW/cm² = 5.14 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) 513 µW/cm² = 5.13 W/m² UVB (EU) ( 280 nm - 315 nm) 18.1 µW/cm² = 0.181 W/m² UVB (US) ( 280 nm - 320 nm) 22.6 µW/cm² = 0.226 W/m² UVA+B ( 280 nm - 380 nm) 161 µW/cm² = 1.61 W/m² Solar UVB ( 290 nm - 315 nm) 18.1 µW/cm² = 0.181 W/m² UVA D3 regulating ( 315 nm - 335 nm) 13.4 µW/cm² = 0.134 W/m² UVA (EU) ( 315 nm - 380 nm) 143 µW/cm² = 1.43 W/m² UVA2 (medical definition) ( 320 nm - 340 nm) 21.7 µW/cm² = 0.217 W/m² UVA (US) ( 320 nm - 380 nm) 139 µW/cm² = 1.39 W/m² UVA1 (variant) ( 335 nm - 380 nm) 130 µW/cm² = 1.3 W/m² UVA1 (medical) ( 340 nm - 400 nm) 123 µW/cm² = 1.23 W/m² vis. UVA ( 350 nm - 380 nm) 102 µW/cm² = 1.02 W/m² VIS Rep3 ( 350 nm - 600 nm) 382 µW/cm² = 3.82 W/m² VIS Rep4 ( 350 nm - 700 nm) 447 µW/cm² = 4.47 W/m² purple ( 380 nm - 420 nm) 7.44 µW/cm² = 0.0744 W/m² VIS ( 380 nm - 780 nm) 350 µW/cm² = 3.5 W/m² VIS2 ( 400 nm - 680 nm) 335 µW/cm² = 3.35 W/m² PAR ( 400 nm - 700 nm) 339 µW/cm² = 3.39 W/m² tmp ( 400 nm - 1100 nm) 346 µW/cm² = 3.46 W/m² blue ( 420 nm - 490 nm) 102 µW/cm² = 1.02 W/m² green ( 490 nm - 575 nm) 132 µW/cm² = 1.32 W/m² yellow ( 575 nm - 585 nm) 16.2 µW/cm² = 0.162 W/m² orange ( 585 nm - 650 nm) 72.2 µW/cm² = 0.722 W/m² red ( 650 nm - 780 nm) 20 µW/cm² = 0.2 W/m² IRA ( 700 nm - 1400 nm) 7.13 µW/cm² = 0.0713 W/m² IR2 ( 720 nm - 1100 nm) 5.07 µW/cm² = 0.0507 W/m² IRB ( 1400 nm - 3000 nm) 0 µW/cm² = 0 W/m²
Actionspectra
Erythema 1.35 UV-Index Pyrimidine dimerization of DNA 11.9 µW/cm² Photoceratitis 2.06 µW/cm² Photoconjunctivitis 0.0378 µW/cm² DNA Damage 0.126 Vitamin D3 6.32 µW/cm² Photosynthesis 227 µW/cm² Luminosity 1140 lx Human L-Cone 169 µW/cm² Human M-Cone 147 µW/cm² Human S-Cone 86.1 µW/cm² CIE X 147 µW/cm² CIE Y 160 µW/cm² CIE Z 167 µW/cm² PAR 1520000 mol photons Extinction preD3 29.1 e-3*m²/mol Extinction Tachysterol 96.6 e-3*m²/mol Exctincition PreD3 13300 m²/mol Extinction Lumisterol 6 m²/mol Exctincition Tachysterol 132000 m²/mol Extinction 7DHC 4.73 m²/mol L-Cone 140 µW/cm² M-Cone 140 µW/cm² S-Cone 138 µW/cm² U-Cone 192 µW/cm² UVR - ICNIRP 2004 1.12 Rel Biol Eff Melatonin Supression 118 µW/cm² Blue Light Hazard 91 µW/cm² (79.5 µW/cm² per 1000 lx) CIE 174:2006 PreVit D3 7.21 µW/cm² Lumen Reptil 1260 "pseudo-lx" Vitamin D3 Degradation 4.69 µW/cm² Actinic UV 1.1 µW/cm² (9.64 mW/klm) Exctincition Lumisterol 8130 m²/mol Exctincition 7DHC 6200 m²/mol Exctincition Toxisterols 1860 m²/mol
Broadbandmeters
Solarmeter 6.2 (UVB, pre 2010) 24.7 µW/cm² Solarmeter 6.5 (UV-Index, pre 2010) 1.77 Leybold UVB 19.6 µW/cm² Leybold UVA 94.3 µW/cm² Leybold UVC 0.00121 µW/cm² DeltaOhm UVB 32.3 µW/cm² DeltaOhm UVC 4.03 µW/cm² Vernier UVB 10.6 µW/cm² Vernier UVA 66.3 µW/cm² Gröbel UVA 114 µW/cm² Gröbel UVB 12.5 µW/cm² Gröbel UVC -0.00317 µW/cm² Luxmeter 1190 lx Solarmeter 6.4 (D3) 5.53 IU/min UVX-31 39.4 µW/cm² IL UVB 0.0111 µW/cm² IL UVA 121 µW/cm² Solarmeter 6.5 (UVI, post 2010) 1.43 UV-Index Solarmeter 6.2 (UVB, post 2010) 13.7 µW/cm² (Solarmeter Ratio = 9.6) Solarmeter AlGaN 6.5 UVI sensor 15.9 UV Index GenUV 7.1 UV-Index 0.804 UV-Index Solarmeter 10.0 (Global Power) (manuf.) 4.36 W/m² Solarmeter 4.0 (UVA) 1.63 mW/cm² LS122 (manuf.) 0.00788 W/m² ISM400 (first guess) 2.56 W/m² LS122 (assumption) 0.127 W/m² ISM400_new 2.01 W/m² Solarmeter 10.0 (Global Power) (assumption) 3.87 W/m²