Sunday, 6 August 2017

Human Eye Sensitivity over the whole Visible spectrum

Human Eye  

   The recipient of the light emitted by most visible-spectrum LEDs is the human eye. Figure 16.1 (a) shows a schematic illustration of the human eye (Encyclopedia Britannica, 1994).

                                          
                                               Fig 16.1. Light receptors of the human eye

   The inside of the eyeball is clad by the retina, which is the light-sensitive part of the eye. The illustration also shows the Fovea (Yellow spot), a cone-rich central region of the retina which affords the high acuteness of central vision. Figure 16.1 (b) shows the cell structure of the retina including the light-sensitive rod cells and cone cells. Also shown are the ganglion cells and nerve fibers that transmit the visual information to the brain. Rod cells are more abundant and more light sensitive than cone cells. Rods are sensitive over the entire visible spectrum. There are three types of cone cells, namely cone cells sensitive in the Red, Green, and Blue spectral range.

Human Eye Sensitivity to Different Lights

Three different vision regimes are shown in Fig. 16.2 along with the receptors relevant to each of the regimes (Osram Sylvania, 2000). Photopic vision relates to human vision at high ambient light levels (e.g. during daylight conditions) when vision is mediated by the cones. The photopic vision regime applies to luminance levels > 3 cd/m2. Scotopic vision relates to human vision at low ambient light levels (e.g. at night) when vision is mediated by rods. Rods have a much higher sensitivity than the cones. However, the sense of color is essentially lost in the scotopic vision regime. At low light levels such as in a moonless night, objects lose their colours and only appear to have different gray levels. The scotopic vision regime applies to luminance
levels < 0.003 cd/m2. Mesopic vision relates to light levels between the photopic and scotopic vision regime (0.003 cd/m2 < mesopic luminance < 3 cd/m2).
The approximate spectral sensitivity functions of the rods and three types or cones are shown
in Fig. 16.3 (Dowling, 1987). Inspection of the figure reveals that night-time vision (scotopic
vision) is weaker in the red spectral range and thus stronger in the blue spectral range as
compared to day-time vision (photopic vision). The following discussion mostly relates to the
photopic vision regime.















Eye Sensitivity Function

The conversion between radiometric and photometric units is provided by the luminous efficiency function or eye sensitivity function, V(λ). In 1924, the CIE introduced the photopic eye sensitivity function V(λ) for point-like light sources where the viewer angle is 2° (CIE, 1931). This function is referred to as the CIE 1931 V(λ) function. It is the current photometric standard in the United States. A modified V(λ) function was introduced by Judd and Vos in 1978 (Vos, 1978; Wyszecki and Stiles, 1982, 2000) and this modified function is here referred to as the CIE 1978 V(λ) function. The modification was motivated by the underestimation of the human eye sensitivity in the blue and violet spectral region by the CIE 1931 V(λ) function. The modified function V(λ) has higher values in the spectral region below 460 nm. The CIE has endorsed the CIE 1978 V(λ) function by stating “the spectral luminous efficiency function for a point source may be adequately represented by the Judd modified V(λ) function” (CIE, 1988) and “the Judd modified
V(λ) function would be the preferred function in those conditions where luminance measurements of short wavelengths consistent with color normal observers is desired” (CIE, 1990).

    The CIE 1931 V(λ) function and the CIE 1978 V(λ) function are shown in Fig. 16.6. The photopic eye sensitivity function has maximum sensitivity in the green spectral range at 555 nm, where V(λ) has a value of unity, i.e. V(555 nm) = 1. Inspection of the figure also reveals that the CIE 1931 V(λ) function underestimated the eye sensitivity in the blue spectral range (λ < 460 nm). Also shown in Fig. 16.6 is the scotopic eye sensitivity function V ′(λ). The peak sensitivity in the scotopic vision regime occurs at 507 nm. This value is markedly shorter than the peak sensitivity in the photopic vision regime.
    
   Note that even though the CIE 1978 V(λ) function is preferable, it is not the standard, mostly
for practical reasons such as possible ambiguities created by changing standards. Wyszecki and
Stiles (2000) note that even though the CIE 1978 V(λ) function is not a standard, it has been used
in several visual studies. The CIE 1978 V(λ) function, which can be considered the most accurate
description of the eye sensitivity in the photopic vision regime, is shown in Fig. 16.7.






























   The eye sensitivity function has been determined by the minimum flicker method, which is the classic method for luminance comparison and for the determination of V(λ). The stimulus is a light-emitting small circular area, alternatingly illuminated (with a frequency of 15 Hz) with the standard color and the comparison color. Since the hue-fusion frequency is lower than 15 Hz, the hues fuse. However, the brightness-fusion frequency is higher than 15 Hz and thus if the two colors differ in brightness, then there will be visible flicker. The human subject’s task is to adjust the target color until the flicker is minimal. Any desired chromaticity can be obtained with an infinite variety of spectral power distributions P(λ). One of these distributions has the greatest possible luminous efficacy. This limit can be obtained in only one way, namely by the mixture of suitable intensities emitted by two monochromatic sources (MacAdam, 1950). The maximum attainable luminous efficacy obtained with a single monochromatic pair of emitters is shown in Fig. 16.8. The maximum luminous efficacy of white light depends on the color temperature; it is about 420 lm/W for a color temperature of 6500 K and can exceed 500 lm/W for lower color temperatures. The exact
value depends on the exact location within the white area of the chromaticity diagram.
For wavelengths ranging from 390 to 720 nm, the eye sensitivity function V(λ) is greater than 10–3. Although the human eye is sensitive to light with wavelengths < 390 nm and > 720 nm, the sensitivity at these wavelengths is extremely low. Therefore, the wavelength range 390 nm ≤ λ ≤ 720 nm can be considered the visible wavelength range. The relationship between color and wavelength within the visible wavelength range is given in Table 16.5. This relationship is valid for monochromatic or near-monochromatic light sources such as LEDs. Note that color is, to some extent, a subjective quantity. Also note that the transition between
different colors is continuous.

Wednesday, 12 July 2017

Measuring Light : Origin of Candela and Lumens

Candela

a) Origin

The candela (symbol : cd) is the SI base unit of luminous intensity; that is, luminous power per unit solid angle emitted by a point light source in a particular direction. The word candela means candle in Latin. A common candle emits light with roughly 1 cd luminous intensity.

 


b) History

Before 1948, there were various standards in various countries for luminous intensity measurement, typically based on the brightness of flame from a "standard candle" of defined composition, or the brightness of an incandescent filament of specific design, one of them being candlepower, used in England. 1 candlepower was the light produced by a pure spermaceti candle weighing 1/6th of a pound and burning at a rate of 120 grains per hour. Another was Hefnerkerze, a unit based on the output of a Hefner lamp. This was used in Germany, Austria and Scandinavia.

After this Jules Violle had proposed a standard based on the light emitted by 1 cm2 of platinum at its melting point (or freezing point), calling this the Violle. The light intensity was due to the Planck radiator (a black body) effect, and was thus independent of the construction of the device. This made it easy for anyone to measure the standard, as high-purity platinum was widely available and easily prepared. The International Commission on Illumination and the CIPM proposed a “new candle” based on this basic concept. However, in the year 1946 the value of the new unit was chosen to make it similar to the earlier unit candlepower by dividing the Violle by 60. The value of the new candle is such that the brightness of the full radiator at the temperature of solidification of platinum is 60 new candles per cm2.

It was then ratified in 1948 by the 9th CGPM which adopted a new name for this unit, the candela. In 1967 the 13th CGPM removed the term "new candle" and gave an amended version of the candela definition, specifying the atmospheric pressure applied to the freezing platinum:
The candela is the luminous intensity, in the perpendicular direction, of a surface of 1 / 600 000 square metre of a black body at the temperature of freezing platinum under a pressure of 101 325 newtons per square metre.
In 1979, because of the difficulties in realizing a Planck radiator at high temperatures and the new possibilities offered by radiometry, the 16th CGPM adopted the modern definition of the candela. The arbitrary (1/683) term was chosen so that the new definition would exactly match the old definition. Although the candela is now defined in terms of the second (an SI base unit) and the watt (a derived SI unit), the candela remains a base unit of the SI system, by definition.

c) Definition

 The candela is the luminous intensity, in a given direction, of a source that emits monochromatic radiation of frequency 540×1012 hertz and that has a radiant intensity in that direction of 1683 watt per steradian.

d) Explanation

 The human eye is most sensitive to a frequency in the visible spectrum near green (wavelength of 555 nanometres), when adapted for bright conditions. More radiant intensity is needed to achieve the same luminous intensity for other frequencies. The luminous intensity for light of a particular wavelength λ is given by
           Iv(λ) =683.002 lm/W.ȳ(λ).Ie(λ)

where Iv(λ) is the luminous intensity in candelas,
          lm is short for lumen,
          W for watt,
           Ie(λ) is the radiant intensity in W/sr and
    ȳ(λ) is the standard luminosity function (photopic).

If more than one wavelength is present (as is usually the case), one must sum or integrate over the spectrum of wavelengths present to get the total luminous intensity.

Lumens and Lux 

a) Introduction

Lumen (symbol: lm) is the SI derived unit of luminous flux. It measures the total quantity of visible light emitted by a source. Power or radiant flux includes all electromagnetic waves emitted, while luminous flux is weighted according to a luminosity function of the human eye's sensitivity to various wavelengths.       
                        (Full moon=1 lux, Direct sunlight=100000lux) 
Relationship between lumens and lux is:-
          1 lux = 1 lm/m2

The lumen is defined in relation to the candela as
          1 lm = 1 cd ⋅ sr.

A whole sphere has a solid angle of 4π steradians, so an isotropic light source has a total luminous flux of
          1 cd × 4π sr = 4π cd⋅sr ≈ 12.57 lumens.

 


b) Lighting

Lamps used for lighting are commonly labelled with their light output in lumens; this is required by law in many places.
A 23 W spiral compact fluorescent lamp (CFL) emits about 1,400–1,600 lm. Many CFL lamps, LED lamps and other alternative light sources are labelled as being equivalent to an incandescent bulb with a specific (generally higher) wattage. Below is a table that shows typical luminous flux for common incandescent bulbs and their equivalents.



Electrical power equivalents for differing lamps

Minimum light output (lumens)
Electrical power consumption (watts)

120 V Incandescent
CFL
LED

200
25W
3-5W
3W

450
40W
9–11W
5–8W

800
60W
13–15W
8–12W

1,100
75W
18–20W
10–16W

1,600
100W
24–28W
14–17W

2,400
150W
30–52W
24-30W

3,100
200W
49–75W
32W

4,000
300W
75–100W
40.5W



c) Explanation

   If a light source emits 1 candela of luminous intensity uniformly across a solid angle of 1 steradian, the total luminous flux emitted into that angle is 1 lumen (1 cd·1 sr = 1 lm). Alternatively, an isotropic 1 candela     light-source emits a total luminous flux of exactly 4π lumens. If the source were partly covered by an ideal absorbing hemisphere, that system would radiate half the luminous flux—only 2π lumens. The luminous intensity would still be 1 candela in those directions that are not obscured.
   The lumen can be taken as a measure of the total amount of visible light in some defined angle, or emitted from some source. The number of candelas or lumens from a source also depends on its spectrum, via the nominal response of the human eye as represented in the luminosity function.
   The difference between the units lumen and lux is that the lux takes into account the area over which the luminous flux is spread. A flux of 1000 lumens, concentrated into an area of one square metre, lights up that square metre with an illuminance of 1000 lux. The same 1000 lumens, spread out over 10m2, produces a dimmer illuminance of only 100 lux. Mathematically, 1 lux = 1 lm/m2.
    A source radiating a power of 1 watt of light in the color for which the eye is most efficient (a wavelength of 555 nm, in the green region of the visible spectrum) has luminous flux of 683 lumens. So a lumen represents at least 1/683 watts of visible light power, depending on the spectral distribution.
    The luminance of a surface source (i.e. a source with a non-zero light-emitting surface area such as a display or an LED) is the ratio of the luminous intensity emitted in a certain direction (measured in cd) divided by the projected surface area in that direction (measured in m2). The luminance is measured in units of cd/m2. In most cases, the direction of interest is normal to the chip surface. In this case, the luminance is the luminous intensity emitted along the chip-normal direction divided by the chip area.
     The projected surface area mentioned above follows a cosine law, i.e. the projected area is given by



                                  Aprojected = Asurface cos Θ 

      where Θ is the angle between the direction considered and the surface normal. This is known as Lambert's cosine law. The light-emitting surface area and the projected area are shown in the figure below.


For LEDs, it is desirable to maximize luminous intensity and luminous flux while keeping the LED chip area minimal. Thus the luminance is a measure of how efficiently the valuable semiconductor wafer area is used to attain, at a given injection current, a certain luminous intensity.

Human Eye Sensitivity over the whole Visible spectrum

Human Eye      The recipient of the light emitted by most visible-spectrum LEDs is the human eye. Figure 16.1 (a) shows a schematic illus...