The invention relates to amalgam spheres for introducing mercury into modern energy-saving lamps.
Modern energy-saving lamps of the TFL (tube fluorescent lamp) or CFL type (compact fluorescent lamp) type belong to the group of low-pressure gas discharge lamps. They comprise a gas discharge bulb which is filled with a mixture of mercury vapour and argon and is coated on the inside with a fluorescent luminophore. The ultraviolet radiation emitted by the mercury during operation is converted by the luminophore coating into visible light by means of fluorescence. The lamps are therefore also referred to as fluorescent lamps.
The mercury required for operation of the lamps was in the past introduced as liquid metal into the gas discharge bulbs. However, introduction of the mercury in the form of amalgam spheres into the gas discharge bulbs has been known for a long time. This makes the handling of the toxic mercury easier and increases the accuracy of metering.
U.S. Pat. No. 4,145,634 describes the use of amalgam pellets which contain 36 atom % of indium and, owing to the high mercury content, contain a large proportion of liquid even at room temperature. The pellets therefore tend to conglutinate when they come into contact with one another. This can be prevented by coating the pellets with suitable materials in powder form. Stable metal oxides (titanium oxide, zirconium oxide, silicon dioxide, magnesium oxide and aluminium oxide), graphite, glass powder, phosphors, borax, antimony oxide and metal powders which do not form an amalgam with mercury (aluminium, iron and chromium) are proposed.
WO 94/18692 describes the use of pellets of zinc amalgam containing from 5 to 60% by weight, preferably from 40 to 60% by weight, of mercury. To produce spheroidal amalgam pellets, the process described in U.S. Pat. No. 4,216,178, in which the molten amalgam is broken up into small droplets by means of a vibrationally excited discharge nozzle and cooled in a cooling medium to below the solidification temperature, is employed.
The pellets are not coated as described in WO 94/18692.
To produce amalgam spheres from the melt, the amalgam has to be heated to a temperature at which the amalgam is completely molten. In the case of a zinc amalgam, this is ensured reliably only at a temperature above 420° C. These high processing temperatures result in a high vapour pressure of mercury and make appropriate safety precautions necessary because of the toxicity of mercury.
JP 2000251836 describes the use of amalgam pellets of tin amalgam for the production of fluorescent lamps. The tin amalgam preferably has only a low mercury content with a tin/mercury atom ratio of 90-80:10-20. This corresponds to a mercury content of from 15.8 to 29.7% by weight. JP 2000251836 gives no information as to how spherical pellets are produced from the amalgam.
A disadvantage of the tin amalgam described in JP 2000251836 is the low mercury content. This makes relatively large amalgam spheres necessary if a particular amount of mercury is to be introduced into the discharge lamps. Owing to the increasing miniaturization which is also being sought in the case of energy-saving lamps, this can lead to problems in the construction and manufacture of the lamps.
It is therefore an object of the invention to provide amalgam spheres of tin amalgam which have a high mercury content and can be reliably stored and used in the production of energy-saving lamps without endangering human health.
This object is achieved by amalgam spheres of a tin amalgam which has a mercury content in the range from 30 to 70% by weight. The amalgam spheres preferably have a mercury content of from 30 to 60% by weight and in particular from 40 to 55% by weight.
The spheres can be produced from a melt of the amalgam by a process described in EP 1381485 B1. For this purpose, the completely molten amalgam is introduced dropwise into a cooling medium having a temperature below the solidification temperature of the amalgam. The temperature of the cooling medium is preferably from 10 to 20° C. below the liquidus temperature of the amalgam. It is advantageous here that tin amalgams melt completely at temperatures below 230° C. The outlay for ensuring occupational hygiene in the production of tin amalgam spheres is therefore considerably lower than in the case of zinc amalgam spheres.
As cooling medium, preference is given to using a mineral oil, an organic oil or a synthetic oil. A silicone oil has been found to be very useful. After formation of the amalgam spheres in the cooling medium, they are separated off from the cooling medium and degreased.
Amalgam spheres having diameters in the range from 50 to 2000 μm, preferably from 500 to 1500 μm, are suitable for the purposes of the invention.
It has been found that liquid phases occur on the surface of the amalgam spheres which have been produced in this way, and the spheres therefore conglutinate during storage and handling if no countermeasures are taken. Conglutination can be prevented by, for example, storing and processing the amalgam spheres at temperatures below 8° C. For storage, a temperature of −18° C. is preferred.
The tendency of the amalgam spheres to conglutinate can be largely suppressed by coating the degreased spheres with a metal or alloy powder which forms an amalgam with mercury. The amalgamation of the metal powder forms a surface layer having a low mercury content on the spheres and since this no longer contains any liquid phases at the usual processing temperatures of the amalgam spheres, it reduces the tendency for conglutination compared to the untreated spheres.
The metal or alloy powder used for the coating should not contain any particles having a particle diameter greater than 100 μm. Particles having larger particle diameters amalgamate only incompletely and lead to a rough surface of the spheres, which makes metering of the spheres more difficult. Preference is given to using a metal or alloy powder whose powder particles have a particle diameter of less than 80 μm. Particular preference is given to metal or alloy powders having an average particle diameter d50 in the range from 5 to 15 μm. Suitable metals have been found to be tin and zinc and alloys of tin or of zinc. Tin or a tin alloy are preferred. Good results have been obtained using alloys of tin with silver and copper, in particular the alloy SnAg3Cu0.5.
To coat the amalgam spheres with the metal or alloy powder, the spheres can, for example, be placed in a rotating vessel and sprinkled with the metal or alloy powder while being continually mixed until conglutination of the spheres can no longer be observed. The amount of metal or alloy powder applied to the amalgam spheres is in the range from 1 to 10% by weight, preferably from 2 to 4% by weight, based on the weight of the amalgam spheres.
A further reduction in the tendency for conglutination is obtained when the amalgam spheres are additionally coated with a powder of a metal oxide in an amount of from 0.001 to 1% by weight, preferably from 0.01 to 0.5% by weight and in particular in an amount of 0.1% by weight, based on the weight of the amalgam spheres, after coating with the metal or alloy powder. The same procedure as for the application of the metal or alloy powder can be employed for this purpose. Suitable metal oxides for the coating are, for example, titanium oxide, zirconium oxide, silicon oxide and aluminium oxide. Preference is given to using an aluminium oxide prepared by flame pyrolysis and having an average particle size of less than 5 μm, preferably less than 1 μm.
The powder layers applied improve the handling of the amalgam spheres in automatic metering machines. The amalgam spheres can stay in such automatic metering machines for an average of up to 3 hours at room temperature before they are introduced into a fluorescent lamp. It has been found here that the amalgam spheres coated with metal or alloy powder and with metal oxide powder withstand the average residence time of 3 hours at temperatures of up to 40° C. in the automatic metering machine without problems. If only one of the two layers is applied, some detachment of the layers applied occurs before the average residence time of 3 hours has elapsed.
The invention is illustrated by the following table. The table shows calculated values for the total mass (Sn+Hg) and the mass of mercury (Hg) of tin amalgam spheres as a function of the diameter of the spheres and for tin amalgams having mercury contents of from 20 to 50% by weight. In addition, the table shows the densities p of the various amalgams as have been used for the calculations.
When spheres of the same diameter are employed, the use of tin amalgam having high mercury contents enables significantly more mercury to be introduced into the gas discharge bulbs than when a tin amalgam having a low mercury content of only 20% by weight is used. Thus, amalgam spheres of SnHg50 containing 50% by weight of mercury contain about three times the mass of mercury as amalgam spheres of SnHg20 containing only 20% by weight of mercury.
Number | Date | Country | Kind |
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07008717.6 | Apr 2007 | EP | regional |
Number | Date | Country | |
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Parent | 12595762 | Jan 2010 | US |
Child | 13929096 | US |