Sodium-vapor lamp

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A sodium vapor lamp

A sodium-vapor lamp is a gas-discharge lamp that uses sodium in an excited state to produce light at a characteristic wavelength near 589 nm.[1]

There are two varieties of such lamps: low pressure and high pressure. Low-pressure sodium lamps are highly efficient electrical light sources, but their yellow light restricts applications to outdoor lighting such as street lamps.[2] High-pressure sodium lamps produce a broader spectrum of light than the low-pressure lamps, but they still have poorer color rendering than other types of lamps.[3] Low-pressure sodium lamps only give monochromatic yellow light and so inhibit color vision at night.

Low-pressure sodium[edit]

An unlit 35 W LPS/SOX lamp
A running 35 W LPS/SOX lamp
Spectrum of a low-pressure sodium lamp. The intense yellow band is the atomic sodium D-line emission, comprising about 90% of the visible light emission for this lamp type.

Low-pressure sodium (LPS) lamps have a borosilicate glass gas discharge tube (arc tube) containing solid sodium, a small amount of neon, and argon gas in a Penning mixture to start the gas discharge. The discharge tube may be linear (SLI lamp)[4] or U-shaped. When the lamp is first started, it emits a dim red/pink light to warm the sodium metal; within a few minutes as the sodium metal vaporizes, the emission becomes the common bright yellow. These lamps produce a virtually monochromatic light averaging a 589.3 nm wavelength (actually two dominant spectral lines very close together at 589.0 and 589.6 nm). The colors of objects illuminated by only this narrow bandwidth are difficult to distinguish.

LPS lamps have an outer glass vacuum envelope around the inner discharge tube for thermal insulation, which improves their efficiency. Earlier LPS lamps had a detachable dewar jacket (SO lamps).[5] Lamps with a permanent vacuum envelope (SOI lamps) were developed to improve thermal insulation.[6] Further improvement was attained by coating the glass envelope with an infrared reflecting layer of indium tin oxide, resulting in SOX lamps.[7]

LPS lamps are among the most efficient electrical light sources when measured in photopic lighting conditions—producing up to 200 lm/W,[8] partly because the light is at a wavelength near the peak sensitivity of the human eye. They are used mainly for outdoor lighting (such as street lights and security lighting) where faithful color rendition is not important. Recent studies show that under typical nighttime mesopic driving conditions, whiter light can provide better results at a lower level of illumination.[9]

LPS lamps are similar to fluorescent lamps in that they are a low-intensity light source with a linear lamp shape. They do not exhibit a bright arc as do High-intensity discharge (HID) lamps; they emit a softer luminous glow, resulting in less glare. Unlike HID lamps, during a voltage dip low-pressure sodium lamps return to full brightness rapidly. LPS lamps are available with power ratings from 10 W up to 180 W; longer bulb lengths can, however, suffer design and engineering problems.

Modern LPS lamps have a service life of about 18,000 hours and do not decline in lumen output with age, though they do increase in energy consumption by about 10% towards end of life. This property contrasts with mercury vapor HID lamps, which become dimmer towards the end of life to the point of being ineffective, while consuming undiminished electrical power.

Light pollution considerations[edit]

For locations where light pollution is a consideration, such as near astronomical observatories or sea turtle nesting beaches, low-pressure sodium is preferred (as in San Jose and Flagstaff, Arizona).[10][11] Such lamps emit light on just two dominant spectral lines (with other much weaker lines), and therefore have the least spectral interference with astronomical observation.[12] The yellow color of low-pressure sodium lamps also leads to the least visual sky glow, due primarily to the Purkinje shift of dark-adapted human vision, causing the eye to be relatively insensitive to the yellow light scattered at low luminance levels in the clear atmosphere.[13][14] One consequence of widespread public lighting is that on cloudy nights, cities with enough lighting are illuminated by light reflected off the clouds. Where sodium vapor lights are the source of urban illumination, the night sky is tinged with orange.

Film special effects[edit]

Sodium vapor process (occasionally referred to as yellowscreen) is a film technique that relies on narrowband characteristics of LPS lamp. Color negative film is typically not sensitive to the yellow light from an LPS lamp, but special black-and-white film is able to record it. Using a special camera, scenes are recorded on two spools simultaneously, one with actors (or other foreground objects) and another that becomes a mask for later combination with different background. This technique originally yielded results superior to blue-screen technology, and was used in years 1956 to 1990, mostly by Disney Studios. Notable examples of films using this technique include Alfred Hitchcock's The Birds and the Disney films Mary Poppins and Bedknobs and Broomsticks.

Later advancements in blue- and green-screen techniques and computer imagery closed that gap, leaving SVP economically impractical.

High-pressure sodium[edit]

High-pressure sodium lamp in operation
Spectrum of high-pressure sodium lamp. The yellow-red band on the left is the atomic sodium D-line emission; the turquoise line is a sodium line that is otherwise quite weak in a low pressure discharge, but becomes intense in a high-pressure discharge. Most of the other green, blue and violet lines arise from mercury.
Diagram showing the spectral output of a typical high-pressure sodium (HPS) lamp.
Office building illuminated by high-pressure sodium lamps.
Office building illuminated by high-pressure sodium lamps.
High-pressure sodium lamp Philips SON-T Master 600 W

High-pressure sodium lamps (sometimes called HPS lights) have been widely used in industrial lighting, especially in large manufacturing facilities, and are commonly used as plant grow lights. They have also been widely used for outdoor area lighting, such as on roadways, parking lots and security areas. Understanding the change in human color vision sensitivity from photopic to mesopic and scotopic is essential for proper planning when designing lighting for roadways.[9]

High-pressure sodium lamps are quite efficient—about 100 lm/W—when measured for photopic lighting conditions. The higher power lamps (600 W) have an efficiency of 150 lm/W.

As the high-pressure sodium arc is extremely chemically reactive, the arc tube is typically made of translucent aluminum oxide. This construction led General Electric to use the tradename "Lucalox" for their line of high-pressure sodium lamps.

Xenon at a low pressure is used as a "starter gas" in the HPS lamp. It has the lowest thermal conductivity and lowest ionization potential of all the non-radioactive noble gases. As a noble gas, it does not interfere with the chemical reactions occurring in the operating lamp. The low thermal conductivity minimizes thermal losses in the lamp while in the operating state, and the low ionization potential causes the breakdown voltage of the gas to be relatively low in the cold state, which allows the lamp to be easily started.

"White" SON[edit]

A variation of the high-pressure sodium introduced in 1986, the White SON has a higher pressure than the typical HPS/SON lamp, producing a color temperature of around 2700 K with a CRI of 85, greatly resembling the color of an incandescent light.[15] These lamps are often used indoors in cafes and restaurants for aesthetic effect. However, white SON lamps have higher purchase cost, shorter life, and lower light efficiency, and cannot compete with HPS at this time.

Theory of operation[edit]

Diagram of a high-pressure sodium lamp.

An amalgam of metallic sodium and mercury lies at the coolest part of the lamp and provides the sodium and mercury vapor that is needed to draw an arc. The temperature of the amalgam is determined to a great extent by lamp power. The higher the lamp power, the higher will be the amalgam temperature. The higher the temperature of the amalgam, the higher will be the mercury and sodium vapor pressures in the lamp and the higher will be the terminal voltage. As the temperature rises, the constant current and increasing voltage consumes increasing energy until the operating level of power is reached. For a given voltage, there are generally three modes of operation:

  1. The lamp is extinguished and no current flows.
  2. The lamp is operating with liquid amalgam in the tube.
  3. The lamp is operating with all amalgam evaporated.

The first and last states are stable, because the lamp resistance is weakly related to the voltage, but the second state is unstable. Any anomalous increase in current will cause an increase in power, causing an increase in amalgam temperature, which will cause a decrease in resistance, which will cause a further increase in current. This will create a runaway effect, and the lamp will jump to the high-current state (#3). Because actual lamps are not designed to handle this much power, this would result in catastrophic failure. Similarly, an anomalous drop in current will drive the lamp to extinction. It is the second state that is the desired operating state of the lamp, because a slow loss of the amalgam over time from a reservoir will have less effect on the characteristics of the lamp than a fully evaporated amalgam. The result is an average lamp life in excess of 20,000 hours.

In practical use, the lamp is powered by an AC voltage source in series with an inductive "ballast" in order to supply a nearly constant current to the lamp, rather than a constant voltage, thus assuring stable operation. The ballast is usually inductive rather than simply being resistive to minimize energy waste from resistance losses. Because the lamp effectively extinguishes at each zero-current point in the AC cycle, the inductive ballast assists in the reignition by providing a voltage spike at the zero-current point.

The light from the lamp consists of atomic emission lines of mercury and sodium, but is dominated by the sodium D-line emission. This line is extremely pressure (resonance) broadened and is also self-reversed because of absorption in the cooler outer layers of the arc, giving the lamp its improved color rendering characteristics. In addition, the red wing of the D-line emission is further pressure broadened by the Van der Waals forces from the mercury atoms in the arc.

End of life[edit]

Sodium vapor street light
Closeup after dark

At end of life, high-pressure sodium (HPS) lamps exhibit a phenomenon known as cycling, caused by a loss of sodium in the arc. Sodium is a highly reactive element and is lost in a reaction with the aluminum oxide of the arc tube. The products are sodium oxide and aluminum:

6 Na + Al2O3 → 3 Na2O + 2 Al

As a result, these lamps can be started at a relatively low voltage, but, as they heat up during operation, the internal gas pressure within the arc tube rises, and more and more voltage is required to maintain the arc discharge. As a lamp gets older, the maintaining voltage for the arc eventually rises to exceed the maximum voltage output by the electrical ballast. As the lamp heats to this point, the arc fails, and the lamp goes out. Eventually, with the arc extinguished, the lamp cools down again, the gas pressure in the arc tube is reduced, and the ballast can once again cause the arc to strike. The effect of this is that the lamp glows for a while and then goes out, typically starting at a pure or bluish white then moving to a red-orange before going out.

More sophisticated ballast designs detect cycling and give up attempting to start the lamp after a few cycles, as the repeated high-voltage ignitions needed to restart the arc reduce the lifetime of the ballast. If power is removed and reapplied, the ballast will make a new series of startup attempts.

LPS lamp failure does not result in cycling; rather, the lamp will simply not strike or will maintain the dull red glow of the start-up phase. In another failure mode, a tiny puncture of the arc tube leaks some of the sodium vapor into the outer vacuum bulb. The sodium condenses and creates a mirror on the outer glass, partially obscuring the arc tube. The lamp often continues operating normally, but much of the light generated is obscured by the sodium coating, providing no illumination.

ANSI HPS ballast codes[edit]

Power output ANSI codes
35 W S76
50 W S68
70 W S62
100 W S54
150 W S55
200 W S66
250 W S50
310 W S67
400 W S51
600 W S106
750 W S111
1000 W S52

See also[edit]


  1. ^ Emsley, John (May 11, 2015). "Sodium: It's salt, soda and street lights, but also much more". Education in Chemistry. Royal Society of Chemistry. Retrieved 2016-11-29. 
  2. ^ Public Works, Department of Public Works (1980). San Jose: Study and report on low-pressure sodium lighting. San Jose: City of San Jose. p. 8. 
  3. ^ Luginbuhl, Christian B. "Low-Pressure Sodium Issues and FAQ". U.S. Naval Observatory Flagstaff Station. US Navy. Retrieved December 5, 2013. 
  4. ^ "SLI/H Sodium". Retrieved 2012-03-03. 
  5. ^ "SO/H Sodium". Retrieved 2012-03-03. 
  6. ^ "SOI/H Sodium". Retrieved 2012-03-03. 
  7. ^ "SOX Sodium". Retrieved 2012-03-03. 
  8. ^ "Why is lightning colored? (gas excitations)". WebExhibits. Retrieved 2007-09-24. 
  9. ^ a b "Mesoptic Street Lighting Demonstration and Evaluation Final Report" (PDF). Lighting research Center, Rensselaer Polytechnic Institute. January 31, 2008. Retrieved 2011-08-29.  (Comparison is with HPS and MH lamps)
  10. ^ "Archived copy" (PDF). Archived from the original (PDF) on 2012-05-15. Retrieved 2012-10-14. 
  11. ^ "Flagstaff Lighting Code" (PDF). Archived from the original (PDF) on 13 September 2014. Retrieved 14 April 2014. 
  12. ^ Luginbuhl, C. B. (12–16 July 1999), "Why Astronomy Needs Low-Pressure Sodium Lighting" (PDF), in R. J. Cohen; W. T. Sullivan, Why Astronomy Needs Low-Pressure Sodium Lighting, Preserving the Astronomical Sky, Proceedings of IAU Symposium 196, Vienna, Austria: International Astronomical Union (published 2001), p. 81 
  13. ^ Luginbuhl, C. B.; Boley, P. A.; Daviws, D. R. (May 2014). "The impact of light source spectral power distribution on sky glow". Journal of Quantitative Spectroscopy and Radiative Transfer. Elsevier. 139: 21–26. doi:10.1016/j.jqsrt.2013.12.004. 
  14. ^ Aubé, M.; Roby, J.; Kocifaj, M. (5 July 2013). "Evaluating Potential Spectral Impacts of Various Artificial Lights on Melatonin Suppression, Photosynthesis, and Star Visibility". PLoS ONE. 8 (7): e67798. doi:10.1371/journal.pone.0067798. PMC 3702543Freely accessible. PMID 23861808. 
  15. ^ "Philips SDW-T High Pressure Sodium White SON". WebExhibits. Retrieved 2007-09-24.