R3111/LEDW455DX1
CRI 90
De flesta av våra produkter finns även tillgängliga i CRI (Ra) 90.
LLMF
The figure that reflects the drop in luminous flux of the light source (LLMF) takes into account failing LEDs, and deterioration of the light output over time. How do we determine this LLMF? We distinguish between the service life of LEDs at the component level and at the luminaire level.
At the component level we take into account the gradual deterioration of the luminous flux of the LEDs (parametric failure or B-lifetime), and the potential breakdown of LEDs (catastrophic failure or C-lifetime). At the luminaire level the complete failure of a luminaire is not relevant (see Luminaire Survival Factor). The LLMF corresponds with the B-lifetime at the luminaire level and hence takes on board the parametric as well as catastrophic failure of the individual LEDs in the luminaires.
In order to achieve an accurate, reliable LLMF for our luminaires, we carry out a ‘principal component analysis’:
- We determine the parametric failure at the component level in accordance with objective LM80/TM21.
- We are unable to calculate the catastrophic failure, but prefer to collaborate with manufacturers who make accurate data available. Whenever no measurement data are offered, we depend on electronic reliability models (MIL-HBK-217F)
UGR
Unified Glare Rating
Detta är en ungefärlig modell som uttrycker risken för bländning.
Standardvärdena sträcker sig från UGR 16 (låg risk för bländning) till UGR 28. I standarden för arbetsbelysning EN12464 införs gränsvärden för UGR för olika rum.
Nedladdningar
Fotometrisk data
- DIALux ULD
- Eulumdat LDT
Specifikationsbeskrivning
- Specifikationsbeskrivning
- Specifikationsbeskrivning med bild
Produktbeskrivning
Produktdatablad
Specifikationsbeskrivning
Produktinformation
Armatur data
Elektrisk data
Power factor
The power factor is a technical indicator of the driver that shows how closely the current of the waveform approximates the sinusoidal reference of the voltage. The power factor (λ) is composed of two parts:
the shift between voltage and current (cos ϕ) and the distortion of the current (harmonics or Total Harmonic Distortion).
The smaller the shift and distortion of the waveform, the fewer losses and pollution on the energy supplier’s distribution network. In ETAP LED drivers we exclusively work with a power factor in excess of 0.9.
Lystid
När strömförsörjningen misslyckas tänds nödbelysningen under en viss tidsperiod: autonomin/lystid, kapacitet?
- 60 minuter: lämplig för de flesta applikationer
- 180 minuter: när evakueringen kräver mer tid, till exempel i höghus eller vårdcentraler
Cirkularitetsindexet
Cirkularitetsindexet
Cirkularitetsindexet visar vilken nivå av cirkularitet och hållbarhet som våra armaturer uppnår.
- Produktens cirkularitetspoäng anger hur väl vår produkt passar in i den cirkulära ekonomin baserat på principerna om oändlighet, enkelhet och utan slöseri.
- Poängen för livstidseffektivitet jämför vår armaturs energi- och materialpåverkan med en referensprodukt på marknaden.
Genom cirkularitetsindexet utmanar vi oss själva att kontinuerligt förbättra våra produkter och uppnå högre poäng när det gäller cirkularitet och hållbarhet. Läs alla detaljer i vår blogg.
Eprel Data ljuskälla
Livstid
Time(hrs) | LLMF(%) | Cx(%) |
---|---|---|
10000 | 99 | 1 |
20000 | 98 | 2 |
30000 | 97 | 3 |
40000 | 96 | 4 |
50000 | 95 | 5 |
60000 | 94 | 6 |
70000 | 93* | 7 |
80000 | 93* | 8 |
90000 | 92* | 9 |
100000 | 91* | 9 |
Måttskiss
Fotometriska data
Ljusstyrka i cd
Gamma | C0 | C45 | C90 | Gamma | C0 | C45 | C90 |
---|---|---|---|---|---|---|---|
0° | 1975.3 | 1975.3 | 1975.3 | 90° | 0.3 | 0.4 | 1.7 |
5° | 1964.9 | 1959.8 | 1958.2 | 95° | 4.2 | 5.9 | 10.2 |
10° | 1929.7 | 1927.5 | 1927.8 | 100° | 16.0 | 22.3 | 31.7 |
15° | 1872.6 | 1869.7 | 1867.0 | 105° | 37.7 | 49.6 | 66.9 |
20° | 1776.1 | 1787.1 | 1788.6 | 110° | 73.8 | 93.8 | 119.6 |
25° | 1651.2 | 1684.3 | 1691.8 | 115° | 130.6 | 158.7 | 187.3 |
30° | 1475.1 | 1539.8 | 1549.9 | 120° | 209.3 | 239.8 | 269.3 |
35° | 1276.3 | 1380.2 | 1370.9 | 125° | 296.9 | 324.2 | 351.2 |
40° | 1049.0 | 1181.5 | 1142.6 | 130° | 380.1 | 394.4 | 416.6 |
45° | 820.0 | 985.6 | 921.1 | 135° | 447.7 | 451.0 | 470.6 |
50° | 574.3 | 772.1 | 681.2 | 140° | 503.1 | 498.7 | 513.1 |
55° | 288.0 | 569.7 | 373.9 | 145° | 542.4 | 542.1 | 549.1 |
60° | 155.8 | 340.9 | 154.0 | 150° | 574.2 | 571.7 | 579.0 |
65° | 38.8 | 127.5 | 89.8 | 155° | 602.3 | 600.8 | 603.5 |
70° | 18.4 | 33.2 | 46.7 | 160° | 623.1 | 622.6 | 623.0 |
75° | 9.9 | 13.8 | 28.9 | 165° | 641.5 | 646.6 | 645.3 |
80° | 1.5 | 5.0 | 14.9 | 170° | 656.7 | 652.4 | 655.8 |
85° | 0.0 | 0.0 | 4.7 | 175° | 663.4 | 664.5 | 664.0 |
90° | 0.3 | 0.4 | 1.7 | 180° | 656.1 | 656.1 | 656.1 |
Luminans
Gamma | C0 | C30 | C45 | C60 | C90 |
45° | 9762 | 11128 | 11732 | 11335 | 10965 |
50° | 7520 | 9381 | 10111 | 9790 | 8921 |
55° | 4227 | 6730 | 8361 | 7886 | 5487 |
60° | 2624 | 4090 | 5739 | 4321 | 2592 |
65° | 773 | 1580 | 2540 | 2029 | 1788 |
70° | 454 | 561 | 816 | 1254 | 1150 |
75° | 321 | 369 | 450 | 695 | 939 |
80° | 72 | 172 | 244 | 353 | 720 |
85° | 0 | 0 | 0 | 37 | 451 |
UGR
Corrected Glare Ratings for a Total Lamp Flux of 5250lm (S = 0.25H)
Room Reflection Factors (%) | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
Ceiling Walls Floor |
70 50 20 |
70 30 20 |
50 50 20 |
50 30 20 |
30 30 20 |
70 50 20 |
70 30 20 |
50 50 20 |
50 30 20 |
30 30 20 |
Room Dimensions | Viewed Crosswise | Viewed Endwise | ||||||||
X = 2H Y = 2H | 15.8 | 16.9 | 16.5 | 17.6 | 18.3 | 16.3 | 17.3 | 17.0 | 18.1 | 18.7 |
Y = 3H | 15.6 | 16.5 | 16.3 | 17.3 | 18.0 | 16.1 | 17.1 | 16.8 | 17.8 | 18.5 |
Y = 4H | 15.5 | 16.3 | 16.2 | 17.1 | 17.8 | 16.0 | 16.9 | 16.8 | 17.7 | 18.4 |
Y = 6H | 15.3 | 16.1 | 16.1 | 16.9 | 17.6 | 15.9 | 16.7 | 16.7 | 17.5 | 18.2 |
Y = 8H | 15.3 | 16.0 | 16.1 | 16.8 | 17.6 | 15.9 | 16.6 | 16.6 | 17.4 | 18.2 |
Y = 12H | 15.2 | 15.9 | 16.0 | 16.7 | 17.5 | 15.8 | 16.5 | 16.6 | 17.3 | 18.1 |
X = 4H Y = 2H | 15.8 | 16.7 | 16.6 | 17.5 | 18.2 | 16.2 | 17.1 | 17.0 | 17.9 | 18.6 |
Y = 3H | 15.6 | 16.4 | 16.4 | 17.1 | 17.9 | 16.1 | 16.8 | 16.9 | 17.6 | 18.4 |
Y = 4H | 15.5 | 16.1 | 16.3 | 16.9 | 17.7 | 16.0 | 16.6 | 16.8 | 17.5 | 18.2 |
Y = 6H | 15.4 | 15.9 | 16.2 | 16.7 | 17.5 | 15.9 | 16.5 | 16.7 | 17.3 | 18.1 |
Y = 8H | 15.3 | 15.8 | 16.1 | 16.6 | 17.4 | 15.9 | 16.4 | 16.7 | 17.2 | 18.0 |
Y = 12H | 15.2 | 15.7 | 16.1 | 16.5 | 17.4 | 15.8 | 16.3 | 16.6 | 17.1 | 17.9 |
X = 8H Y = 4H | 15.3 | 15.8 | 16.1 | 16.7 | 17.5 | 15.8 | 16.3 | 16.7 | 17.2 | 18.0 |
Y = 6H | 15.2 | 15.6 | 16.1 | 16.5 | 17.3 | 15.7 | 16.2 | 16.6 | 17.0 | 17.8 |
Y = 8H | 15.1 | 15.5 | 16.0 | 16.4 | 17.2 | 15.7 | 16.0 | 16.6 | 16.9 | 17.8 |
Y = 12H | 15.0 | 15.4 | 15.9 | 16.3 | 17.1 | 15.6 | 15.9 | 16.5 | 16.8 | 17.7 |
X = 12H Y = 4H | 15.2 | 15.7 | 16.1 | 16.6 | 17.4 | 15.8 | 16.2 | 16.6 | 17.1 | 17.9 |
Y = 6H | 15.1 | 15.5 | 16.0 | 16.4 | 17.2 | 15.7 | 16.0 | 16.5 | 16.9 | 17.8 |
Y = 8H | 15.0 | 15.4 | 15.9 | 16.3 | 17.1 | 15.6 | 15.9 | 16.5 | 16.8 | 17.7 |
UGR Variations with Observer Position for Luminaire Spacings S | ||||||||||
S = 1.0H | +1.1 | -2.3 | +0.7 | -1.5 | ||||||
S = 1.5H | +2.3 | -7.5 | +2.1 | -6.6 | ||||||
S = 2.0H | +3.6 | -14.7 | +3.3 | -8.3 |
Verkningsgrad
Room Reflection Factors (%) | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
Ceiling Walls Floor |
80 50 20 |
80 30 20 |
80 10 20 |
50 50 20 |
50 30 20 |
50 10 20 |
30 50 20 |
30 30 20 |
30 10 20 |
0 0 0 |
RCR = 1 | 101 | 99 | 97 | 85 | 83 | 82 | 75 | 74 | 73 | 61 |
2 | 91 | 87 | 84 | 76 | 74 | 72 | 68 | 66 | 65 | 54 |
3 | 81 | 76 | 73 | 69 | 66 | 63 | 62 | 59 | 57 | 48 |
4 | 73 | 67 | 63 | 63 | 58 | 55 | 56 | 53 | 50 | 42 |
5 | 66 | 60 | 55 | 57 | 52 | 49 | 51 | 48 | 45 | 38 |
6 | 60 | 53 | 49 | 52 | 47 | 43 | 47 | 43 | 40 | 34 |
7 | 55 | 48 | 43 | 48 | 42 | 39 | 43 | 39 | 36 | 31 |
8 | 50 | 43 | 39 | 44 | 39 | 35 | 40 | 36 | 32 | 28 |
9 | 46 | 39 | 35 | 40 | 35 | 32 | 37 | 33 | 30 | 25 |
10 | 43 | 36 | 31 | 37 | 32 | 29 | 34 | 30 | 27 | 23 |
Room Reflection Factors (%) | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
Ceiling Walls Floor |
80 50 30 |
80 30 30 |
80 50 10 |
50 30 10 |
50 50 30 |
50 30 30 |
50 50 10 |
50 30 10 |
30 30 10 |
0 0 0 |
k = 0.60 | 51 | 43 | 49 | 42 | 45 | 39 | 43 | 38 | 36 | 29 |
0.80 | 62 | 54 | 58 | 52 | 54 | 48 | 52 | 47 | 44 | 36 |
1.00 | 70 | 62 | 65 | 59 | 61 | 55 | 58 | 53 | 49 | 41 |
1.25 | 79 | 72 | 73 | 67 | 68 | 63 | 64 | 60 | 56 | 47 |
1.50 | 85 | 78 | 77 | 72 | 73 | 68 | 68 | 64 | 60 | 50 |
2.00 | 92 | 86 | 83 | 78 | 78 | 74 | 72 | 69 | 64 | 54 |
2.50 | 98 | 92 | 86 | 83 | 82 | 78 | 76 | 73 | 67 | 57 |
3.00 | 102 | 97 | 89 | 86 | 85 | 82 | 78 | 76 | 70 | 59 |
4.00 | 106 | 102 | 92 | 89 | 88 | 85 | 80 | 78 | 72 | 61 |
5.00 | 109 | 105 | 94 | 92 | 90 | 88 | 82 | 80 | 73 | 62 |