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Mention of lighting |
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What is light?
Light is a form of energy composed of electromagnetic
waves that spread through space at the speed of
300.000 km per second, all similar, except for
the frequencies, to radio waves.
An electromagnetic radiation is composed of a
magnetic field variable in accordance with sine
curve law.
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The
characteristic dimensions are the maximum value (or
efficiency value) of the intensity of the field and
the light wavelength ( ) which in turn determines the
colour of the light.
In time terms, the wavelength finds equivalence in the
time period (T), the time consumed between two successive
maximum values of homogenous mark. The correlation between
the time period T and the wavelength is obvious, given
that the propagation speed c of electromagnetic waves
through space is known and constant. |
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Luminous
flux |
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Luminous
flux measures the light potency useful in terms of
vision.
Logically it should also be measured in watts, but
the unit used is the lumen (symbol lm). One lumen
corresponds to 1/683 W of yellow light, corresponding
to radiation with a wavelength of 555nm.
Although precise mathematical relationships exist
between lumen and watt, it is important not to confuse
the potency absorbed by electric lightbulbs with the
flow emitted; in fact, only a minimal part of the
potency absorbed is transformed in visible light radiation.
For simplicity, but without respect for the reality
of physical law, light flow is defined as "the
quantity of light emitted by a lightbulb"; thus
said, it is not a question of quantity of energy (joule)
but of potency (watts translated into lumen).
Furthermore it is to be emphasised that it is the
potency transmitted that is weakened when it meets
or crosses means of dissipation.
Thus, the luminous flux emitted by a lighting appliance
is less than that emitted by lightbulb it contains
due to the losses caused by absorption by the reflector
and/or diffusor (concept of appliance output).
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Light
intensity |
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Light
intensity is a dimension that measures the light potency
of rays emitted from the source in a given direction.
In order to understand the concept, with reference to
Figure 3, one can imagine a spherical source, for example
an opaline globe, that diffuses light uniformly in the
entire solid angle of 12.56 sterad (a three-dimensional
angle measured in steradiants). If the total light flow
is, for example, 1000 lumen, in every direction one
achieves a light intensity of 1000:12.56 candles (symbol
cd), that is around 79.57 cd.
Light intensity (symbol l) can in this way be defined
as the infinitesimal relationship between light flow
and the angle at which it is emitted.
Light intensity is measured in candles (that is in lm/sterad).
Sometimes, and not without much confusion, this dimension
is attributed to a lightbulb imagining it as a uniformly
emitted light source: under this hypothesis one candle
is equivalent to 12.56 lumen.
The concept of light intensity is the basis of the entire
calculation of illuminotechnics, based on defined physical
elements (a point per point calculation).
Whilst the flow (minimal weakening apart) is a characteristic
typical of light sources (lightbulbs), intensity is
typical of lighting appliances; for a precise calculation
of illumination it is necessary to know the light intensity
emitted by a lighting appliance on at least two significant
vertical right-angles (photometric indicator).
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IIllumination |
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IIllumination
is mathematically defined as the relationship between
the flow incident to a surface and the surface itself
measured in m2 (lumen/m2=lux). Only the incident flow
should be considered, that is as it hits the surface
on the perpendicular. If the light ray is not perpendicular
to the surface the relationship is multiplied by the
cosine of the angle of incidence with respect to the
vertical.
This first rough concept becomes exact only in the case
of uniform parallel flow (for example sunlight with
respect to a surface of modest dimensions). In general
situations light is diffused by a surface much smaller
than that illuminated and the rays diverge for this
reason. It follows that illumination E decreases in
line with distance squared.
The units of measure (light flow, light intensity, illumination)
are well chosen so that the illumination of a point
is given by the relationship between light intensity
of the incidental ray and the distance squared.
For up to 1 m from the source, illumination is numerically
equal to light intensity of the incident ray. For example
along a ray with an intensity of 100 cd one will find,
respectively:
- up to 1 m 100 lx;
- up to 2 m 25 lx;
- up to 4 m 6,25 lx etc.
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Luminance |
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Taking
a further look, with the human eye, the effect of light
flow, light intensity and illumination can be evaluated
better if the concept of luminance is introduced.
The luminance of a body from which the eye receives
light is defined as the relationship between light intensity
(candela) of the ray that hits the retina and the emitting
surface (m2). Luminance (measurement symbol L) is measured
in nit (symbol nt, dimension cd/m2). |
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Colour |
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Every
wavelength comprised in the range of visible electromagnetic
radiations corresponds to the perception of colour by
the human eye, variable from red (700nm) to blue-violet
(435nm), passing through yellow (570nm).
"Pure" colours, that is formed by a perfect
radiation sine curve, are only theoretical; in reality
the eye, with respect to electromagnetic waves, behaves
like a multi-band antenna in such a way that the colours
are perceived as additional syntheses to monochrome
radiations.
Thus, for example, white does not exist as a primary
colour, but is obtained by a suitable dose of red, green
and yellow.
The colour of sunlight is the same white at which artificial
light is aimed.
If a light source is not able to produce determined
lightwaves in determined doses, the colours of the objects
illuminated are subject to distorsion. |
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Tonality |
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The
artificial light produced by electric lightbulbs is
not perfectly white; it can tend towards red (warm light)
or blue (cold light) if, respectively, there is an abundance
of red or blue radiations.
The method most used to define tonality is that of degrees
Kelvin.
Tonality is normalized by the CIE in three groups according
to the following symbols:
- W up to 3300 K indicate warm tones;
- I from 3300 to 5300 K indicate daylight;
- C over 5300 K indicate cold light.
In the range of tonalities comprised between 3000 and
6000 K colours are perceived correctly thus the choices
are subjective or influenced by special usage (for example
the aspect of flesh improves if illuminated by light
with warm tones; whilst the aspect of fish is better
highlighted by cold tonalities). |
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Chromatic
yield |
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The
chromatic yield of a lightbulb expresses its capacity
to reproduce the natural colours of the objects illuminated.
The colour of such objects depends on the light reflected:
thus, an object appears red because it absorbs all other
radiations and reflects only combinations of monochrome
lights that in synthesis are red.
Without going into complex detail it is fairly evident
that an object is not able to reflect a radiation it
does not receive. Therefore, chromatic yield is perfect
only if artificial light produces the same radiations
as sunlight and in the same doses. This optimal condition
clearly cannot be reached. The level of imperfection
is conventionally measured by a numeric index preceded
by the symbol Ra:
the number 100 indicates the perfection (100% colour
yield) and 0 indicates absolute imperfection (monochromatic
vision).
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Light and
environment |
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| Our modern society requires an increasing quantity of electricity for industry, ...
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