The optimum operating gas pressure for incandescent tungsten filament lamps

Author:

Coaton J.R.1

Affiliation:

1. British Lighting Industries Ltd., Research and Engineering Laboratories, Leicester

Abstract

The life of a tungsten filament incandescent lamp may be increased by raising the gasfilling pressure. However, recent experiments have suggested that beyond a certain point the gain in life is more than offset by the consequential fall in efficacy. This aspect has been investigated theoretically and a formula developed which relates power losses (and hence efficacy) directly to a function of the gasfilling pressure. Calculations for a range of lamps relate changes in life, efficacy and overall quality to changes in gasfilling pressure. The results are supported by the experimental evidence and show that for every lamp design there exists an optimum gasfilling pressure which gives the maximum overall performance. Finally, a general equation has been derived from which the optimum gasfilling pressure can be deduced. The investigation indicates that the performance of many incandescent and tungsten halogen lamps could be improved by adjusting the gasfilling pressure to coincide with the optimum value.

Publisher

SAGE Publications

Subject

Electrical and Electronic Engineering,Atomic and Molecular Physics, and Optics

Cited by 5 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. One Hundred Years of Technical Progress in Light Source Technology;2023 IEEE Sustainable Smart Lighting World Conference & Expo (LS18);2023-06-08

2. Computer simulation of the operating pressure of tungsten halogen lamps;Journal of Physics D: Applied Physics;2005-08-19

3. The life and performance of incandescent lamps;Lighting Research & Technology;1980-06

4. The Life-Voltage Exponent for Tungsten Lamps;Journal of the Illuminating Engineering Society;1973-01

5. The influence of convection and thermal diffusion on halogen separation in vertical burning linear tungsten-halogen lamps;Journal of Physics B: Atomic and Molecular Physics;1971-02

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