Physica Scripta. Vol. T105, 98–100, 2003 UV, Visible and IR Spectrum of the Cs High Pressure Lamp G. Pichler1,, V. Živčec1, R. Beuc1, Ž. Mrzljak2, T. Ban1, H. Skenderović1, K. Günther3 and J. Liu3 1 Institute of Physics, P.O. Box 304, HR-10001 Zagreb, Croatia Factory of Electric Lamps, Zagreb, Croatia 3 OSRAM, Berlin, Germany 2 Received February 21, 2003; accepted February 21, 2003 PACS Ref: 32.70.Fw, 42.72. g, 52.80.Yr Abstract High pressure pulsed discharge with cesium vapor could become a very promising lamp, because of its white light properties. It has considerable losses in the infrared spectral region and negligible contribution in the near UV spectral region. We shall present the results of extensive spectral studies of such a lamp with a special emphasis on the near infrared and near UV portions of emission spectra for a variety of experimental conditions. We shall discuss the origin of atomic emission lines and some peculiar molecular bands, which contribute to the overall emission in these spectral regions. 1. Introduction The history of light sources development is very rich in surprises and novel technological solutions. Since the time electricity became the main driving force of modern light sources several very interesting phases have been seen. From incandescent lamps using carbon filament to tungsten filament is certainly an important early development (Edison, Just and Hanaman, Coolidge). Then the electric discharge lamps received considerable attention mainly because of their much larger efficiency to produce white light. Low and high pressure light sources with different gas and material fillings can nowadays reach between 100 and 200 lumens per watt [1,2]. The highest efficiencies are obtained with low pressure sodium lamps, but they have a very poor color reproduction capability (poor color rendering index, CRI). The high pressure sodium lamps attain better CRI, but their efficiency is typically about 100 lumens per watt. Metal-halogen lamps attain very high CRI factors and have acceptable efficiency. In the modern world approximately 20% of the total electrical energy is used for lighting purposes [3]. It is not surprising to observe several new developments toward more efficient, less toxic, white light sources with excellent CRI factor approaching the value of 100, which can be attained under normal sunshine. High pressure sodium lamps are widely employed light sources for outdoor purposes. However, they have relatively weak blue part of the spectrum and strong absorption in a wide region around the center of the sodium D lines. High sodium pressure causes extended collision-induced line wings which spread into green and red spectral regions. Recently, there was a serious attempt to develop pulsed high-pressure cesium discharge lamps [4,5], but the development went up to almost 50 lm/W efficiency. We shall present a few of the latest spectroscopic results of these high pressure pulsed cesium discharge lamps in order to point to some possible e-mail: [email protected] Physica Scripta T105 directions in the future development of this new alkali light source. 2. Experiment In all our emission measurements we used several different scanning monochromators with appropriate photomultipliers sensitive in ultraviolet, visible and near-infrared spectral regions. The output from the photomultipliers was amplified and processed by a boxcar averager and recorded in a laboratory computer. We found two regions of voltage where the lamp could operate in a stable mode. The first was in the pulsed mode of operation at 220 V. A stable pulsed light signal was achieved for electric currents around 10 A and pulse repetition of about 286 Hz. The second region was at about 110 V where the electric current was around 6 A and the pulse repetition decreased to 170 Hz. As will be shown below, the emission spectra from the lamp at 286 Hz current pulse repetition (voltage 220 V) differs strongly from the emission spectra at 170 Hz current pulse repetition (voltage reduced to 110 V). 3. Results In Fig. 1 we present an overall spectrum at 286 Hz repetition, obtained by a boxcar averager with the gate placed at the maximum of the pulses. The high pressure discharge in the alumina burner of a cesium lamp exhibits a strong spectrum in the visible, and after profound absorption around the cesium resonance lines (800– 960 nm), it also shows considerable emission in the infrared spectral region. At this high electric current all other atomic spectral lines appear almost entirely in absorption. In Fig. 2 a spectrum of the same lamp is shown, but now at a voltage of only 125 V, and pulse repetition of 170 Hz. All atomic spectral lines now appear mostly in emission. There are also some molecular spectral phenomena, which can be attributed to bound excited Cs2 molecules, and some of them require additional studies [6,7,8,9]. A Cs partial energy term diagram is shown in Fig. 3. We denote spectral transitions that have been observed in the lamp emission spectrum at lower running voltage. The transitions from higher energy levels are not explicitly shown, although they can be readily observed in Fig. 4, where we denote their positions by crosses. This portion of the spectrum from 300 to 625 nm, has been taken by means of a 1m McPherson scanning monochromator. The UV portion of the cesium pulsed high-pressure lamp exhibits a few principal series lines of cesium, some forbidden lines # Physica Scripta 2003 UV, Visible and IR Spectrum of the Cs High Pressure Lamp Fig. 1. Overall spectrum of the high-pressure pulsed cesium lamps at higher repetition rate and at voltage of 220 V. Fig. 2. Overall spectrum of high-pressure pulsed cesium lamps at lower repetition rate and at a voltage of 125 V. Fig. 3. Energy term diagram of cesium with a few spectral transitions. (6s-nd and 6s-ns transitions) and accompanying recombination continuum. In the visible part of the spectrum the limits of nd3=2 6p1=2 and nd5=2;3=2 6p3=2 are shown by two vertical lines close to 500 nm. In Fig. 5 we present an interesting comparison between two lamps having different burners, both at 110 V. It appears that the alumina burner (PCA) was much stronger # Physica Scripta 2003 99 Fig. 4. Ultraviolet and portion of the visible spectrum of the cesium lamp at a voltage of 110 V. Fig. 5. Comparison of the overall spectrum of two cesium lamps at 110 V, having a PCA burner of 3 mm in diameter, and a sapphire burner with 5 mm diameter. than the burner made out of pure sapphire crystal. It is certainly the consequence of a narrower cylinder in the case of alumina burner. Maya and coworkers [5] showed that the lamp efficiency increases for decreasing diameter of the burner. This causes stronger plasma constriction, which increases the plasma temperature and thus the light efficiency. Finally, we show what kind of lamp tailoring we need in order to increase the cesium lamp efficiency. We definitely need to cut the near infrared and infrared portions of the spectrum, whereas the blue-green portion should also be a bit more increased. The near infrared part could be efficiently cut away by using a mixture of rubidium and cesium in the burner. The transmission spectrum of dense rubidium vapor exhibits strong resonance line absorption valleys, as shown in Fig. 6. This strong absorption in the spectral region 740–830 nm might presumably increase the mixed Rb-Cs lamp efficiency by about 10–20%. In our future work we shall concentrate on the study of the infrared portion of the pulsed cesium discharge from 1 to 5 microns, in order to assess the losses and eventually to find remedies that will increase the lamp efficacy. Physica Scripta T105 100 G. Pichler et al. Lamp tailoring may include coating of the bulb inner glass walls which enables infrared reflection and transmission of the visible photons (hot mirror). Furthermore, the composition of the arc plasma may be even more complex, adding elements whose strong resonance lines may enrich certain parts of the visible spectrum. We believe that better energy saving may be achieved and with lower light pollution, mainly because of pulsed mode of lamp operation. 5. Conclusion Fig. 6. Transmission spectrum of dense rubidium vapor at a temperature of about 350 C, where the strong and broad absorption of the first resonance rubidium lines is readily visible. 4. Discussion It is interesting that we found two stable regimes of the high pressure pulsed cesium discharge having entirely different spectra. At a current of 10 A and repetition rate of 286 Hz, the cesium lamp of 80 W has a temperature of about 3850 K, and the visible radiation can be fitted to a black-body radiation curve. However, the lamp efficacy was only up to 45 lm/W. On the other hand, the color rendering index (CRI) is very high and can reach values above 98. The radiance in the ultraviolet is almost negligible and there are no relevant dangerous substances that could enter the environment by recycling. Changes in the input voltage do not influence much the CRI factor, and therefore it possesses excellent dimming properties [5]. However, the infrared spectrum might appear much more sensitive to voltage changes than the visible part. We found one satellite band peaking at 945 nm, a second peaking at 980 nm and a third peaking at 1055 nm. These observations have been performed for burners made of PCA and pure sapphire. We calculated the profiles of these infrared satellite bands using ab initio potential curves with appropriate transition dipole moments and found interesting correspondence with observed infrared satellite bands. Several avoided crossings at shorter interatomic distances could only be observed in emission since they lie above the repulsive lowest triplet potential energy curve [10]. High pressure pulsed cesium lamp offers interesting subjects for the study of atomic and molecular spectral features at large atom densities and elevated temperatures, especially when the current is about 6 A and the repetition rate falls to 170 Hz only. The light intensity depends on the diameter of the burner, and in the case of PCA burner it was about 3 mm, whereas for the sapphire burner it was about 5 mm. The smaller the diameter of the burner the stronger is the emission because of the tighter constriction of the discharge plasma. It would be of considerable interest to further study even smaller constrictions in special capillary cesium discharges. Physica Scripta T105 The endeavor to increase the pulsed cesium lamp efficiency, will certainly contribute to better energy savings, better color rendering index, and less toxic plasma composition. However, bright, white and efficient new light sources may contribute to so-called light pollution. Changing the dark nights into illuminated surfaces of modern cities leads to many changes in the natural life of the planet. Pulsed lamp regime may be used to diminish light pollution by means of appropriate switching according to the need for illumination of certain streets, bridges etc. only when traffic is present. For entirely new light sources we definitely need ideas that may be extracted from the vast body of atomic and plasma physics, but also from solid state physics [11] European Cost 529 project under the title ‘‘Lighting for the 21st century’’ will eventually transform into a Network of Excellence within the Framework 6 Program. We may expect that new light sources will emerge in the near future with unprecedented efficacy in excess of 200 lm/W. Acknowledgement This work was supported by the Ministry of Science and Technology of the Republic of Croatia (Projects 0035002 and 0035004) and by OSRAM GmbH, Berlin. This work is also connected with COST 529: Light Sources for the 21st century. References 1. Waymouth, J. F., ‘‘Electric Discharge Lamps,’’ (Cambridge, MIT Press, 1971). 2. De Groot, J. J. and Van Vliet, J. A. J. M., ‘‘The High-Pressure Sodium Lamps,’’ (Philips Technical Library, Scholium Intl., 1986). 3. Born, M. and Jüstel, T., Physik Journal 2, 43 (2003). 4. Liu, J., Günther, K., Kaase, H. and Serick, F., Proc. 8th Int. Symp. Science and Technology of Light Sources (Greifswald, Germany, 1998) paper CO2. 5. Gu, H., Muzeroll, M. E., Chamberlain, J. C. and Maya, J., Plasma Sources Sci. Technol. 10, 1 (2001). 6. Ban, T., Skenderović, H., Ter-Avetisyan, S. and Pichler, G., Appl. Phys. B 72, 337 (2001). 7. Ban, T. et al., Chem. Phys. Lett. 345, 423 (2001). 8. Dion, C. M. et al., European Phys. J. D, 18, 365 (2002). 9. Ban, T., Skenderović, H., Beuc, R., Veža, D. and Pichler, G., European Phys. J. D 25, 209 (2001). 10. Ban, T., Skenderović, H., Beuc, R. and Pichler, G., Europhys. Lett. 48, 378 (1999). 11. Zukauskas, A., Shur, M. S. and Caska, R. ‘‘Introduction to SolidState Lighting,’’ (Wiley, New York, 2002). # Physica Scripta 2003
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