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2017 | 13 |

Tytuł artykułu

Cooling-times of tungsten filament lamps

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Treść / Zawartość

Warianty tytułu

Języki publikacji

EN

Abstrakty

EN
During steady-state operation, hot-coiled filaments in incandescent lamps provide luminous flux for illumination, but when switched off, the temperature, as well as the light output drops quite fast. The cooling-time of a lamp is the time required for the hot filament to cool down to ten per cent light output after the circuit is opened. In this paper, the exercise of estimating luminous flux and coolingtimes for typical 10, 100, 500 and 1000 W lamps has been undertaken for the first time for the benefit of students. This problem involves three disciplines: electricity, optics and heat. Information drawn from field of Electrical studies allows us to understand the power that quickly heats the filament, followed by that from optics that helps us in determining the light output, while heat studies are responsible for understanding the cooling of the hot filament. This last is largely explained through the Stefan-Boltzmann law. In this paper, we show that the supposition of linear configurations for the filaments neither matches luminous flux nor the cooling-times. Both fall short. H.S. Leff’s suggestion of introducing a shadow factor that reduces the exposed surface area, as it so happens in the coiled filaments, successfully explains the measured observations.

Słowa kluczowe

Wydawca

-

Rocznik

Tom

13

Opis fizyczny

p.52-62,ref.

Twórcy

autor
  • Department of Farm Engineering, Banaras Hindu University, Varanasi 221005, India

Bibliografia

  • [1] Incandescent Lamps, Pamphlet TP-110R2 (Nela Park, OH: General Electric Company, 1984) pp. 35, 24
  • [2] The incandescent lamps discussed in the above “bulletin are those that are commonly referred to as “large” lamps. This designation does not necessarily imply large physical size, but refers, usually, to lamps that are operated on standard-voltage circuits, universally found in residential, commercial, and industrial use.” p. 2 in the ref. 1
  • [3] Harvey S. Leff., Illuminating physics with light bulbs, Phys. Teach 28, 30-35 (1990).
  • [4] H. A. Jones and Irving Langmuir, The characteristics of tungsten filaments as functions of temperature: Part II, Gen. Electr. Rev. 30,354-361 (July 1937)
  • [5] M. R. Vukcevich, The Science of Incandescence, (Advanced Technology Department, GE Lighting, Nela Park, Cleveland, 1992), Chapter 9.
  • [6] D. C. Agrawal, H. S. Leff, and V. J. Menon, Efficiency and efficacy of incandescent lamps, Am. J. Phys. 64, 649- 654 (1996)
  • [7] D. C. Agrawal, Moon, Super-Moon, Planets of the Solar System and Star Vega: Brightness and Size. J Phys Astron. 5, 1-20 (2017).
  • [8] R. D. Larrabee, The spectral emissivity and optical properties of tungsten. Technical Report 328, (Research Laboratory of Electronics, MIT, Cambridge, Mass, May 21, 1957)
  • [9] W. H. Stephen and Chun T. Wang Tungsten Sources, Metallurgy, Properties and Applications ( Plenum, New York, 1979) chapter 6
  • [10] W. S. Wagner, Temperature and color of incandescent lamps, Phys. Teach 29, 176-177 (1991).
  • [11] V. J. Menon, and D. C. Agrawal, Lifetimes of incandescent bulbs, Phys. Teach 41, 100-101 (2003).
  • [12] V. J. Menon, and D. C. Agrawal, A theory for the mortality curve of filament lamps, Jour. Mater. Engg. Perf. 16, 1-6 (2007).
  • [13] D. C. Agrawal,and V. J. Menon, Light bulb exponent-rules for the classroom, IEEE Trans. Educ. 43, 262-265 (2000).

Typ dokumentu

Bibliografia

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