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You must consent to the activation of permanent cookies. Precise engineered ridged linear fixture with IP68 for pool lighting and water features with challenging requirements.
Especially designed for long homogeneous linear light lines to create a pleasant atmosphere within and around the pool area and accentuate the elements of design.
Invincible by skill - invisible by design. The updated IP classification now stretch to IP67, meaning water resistance and suitable for canopied outdoor use.
Flexible IP67 luminaires offering various illuminated surfaces and bending directions. Each of them uses polyurethane encapsulation material offering a premium waterproof sealing, UV resistance, chemical stability against urban gazes and protection against abrasion damages.
Light lines bendable in one direction top view or side view with a perfectly homogeneous and dot-free light surface for outdoor architectural lighting.
Pixelized light line produced to the desired length with IP67 connectors on both ends for fast indirect facade lighting installations. Field cuttable light line with visible pixels and high efficiency ideal for indirect lighting applications.
Modular luminaire with 8 different optics available and side cabling and a large panel of mounting options. Sleek design luminaire for general lighting manufactured to length.
Available as pendant, surface and recessed. Pixelized light line produced to the desired length with IP67 connectors on both ends for fast indirect facade lighting installations.
Suitable with 10 different optics. To protect your personal information, the connection to YouTube has been blocked.
Be grateful and live each day to the fullest. So shines a good deed in a weary world. Le Guin. One does not become enlightened by imagining figures of light, but by making the darkness conscious.
Some people without possessing genius have a remarkable power of stimulating it. Choose a place where you won't do harm - yes, choose a place where you won't do very much harm, and stand in it for all you are worth, facing the sunshine.
Forster, A Room with a View. Each photon emitted will be "red"- or "blue"-shifted by the Doppler effect depending on the velocity of the atom relative to the observer.
The higher the temperature of the gas, the wider the distribution of velocities in the gas. Since the spectral line is a combination of all of the emitted radiation, the higher the temperature of the gas, the broader the spectral line emitted from that gas.
This broadening effect is described by a Gaussian profile and there is no associated shift. The presence of nearby particles will affect the radiation emitted by an individual particle.
There are two limiting cases by which this occurs:. Inhomogeneous broadening is a general term for broadening because some emitting particles are in a different local environment from others, and therefore emit at a different frequency.
This term is used especially for solids, where surfaces, grain boundaries, and stoichiometry variations can create a variety of local environments for a given atom to occupy.
In liquids, the effects of inhomogeneous broadening is sometimes reduced by a process called motional narrowing. Certain types of broadening are the result of conditions over a large region of space rather than simply upon conditions that are local to the emitting particle.
Electromagnetic radiation emitted at a particular point in space can be reabsorbed as it travels through space. This absorption depends on wavelength.
The line is broadened because the photons at the line center have a greater reabsorption probability than the photons at the line wings.
Indeed, the reabsorption near the line center may be so great as to cause a self reversal in which the intensity at the center of the line is less than in the wings.
This process is also sometimes called self-absorption. Radiation emitted by a moving source is subject to Doppler shift due to a finite line-of-sight velocity projection.
If different parts of the emitting body have different velocities along the line of sight , the resulting line will be broadened, with the line width proportional to the width of the velocity distribution.
For example, radiation emitted from a distant rotating body, such as a star , will be broadened due to the line-of-sight variations in velocity on opposite sides of the star.
The greater the rate of rotation, the broader the line. Another example is an imploding plasma shell in a Z-pinch. Radiative broadening of the spectral absorption profile occurs because the on-resonance absorption in the center of the profile is saturated at much lower intensities than the off-resonant wings.
Therefore, as intensity rises, absorption in the wings rises faster than absorption in the center, leading to a broadening of the profile.
Radiative broadening occurs even at very low light intensities. Each of these mechanisms can act in isolation or in combination with others.