Home > Research > Publications & Outputs > Absolute optical calibration using a simple tun...

Electronic data

View graph of relations

Absolute optical calibration using a simple tungsten light bulb: Experiment

Research output: Contribution to conference - Without ISBN/ISSN Other

Published

Standard

Absolute optical calibration using a simple tungsten light bulb: Experiment. / Kosch, M. J.; Mäkinen, S.; Sigernes, F. et al.
2003. 50-54 Proceedings of the 30th Annual European Meeting on Atmospheric Studies by Optical Methods.

Research output: Contribution to conference - Without ISBN/ISSN Other

Harvard

Kosch, MJ, Mäkinen, S, Sigernes, F, Harang, O, Sigernes, F (ed.) & Lorentzen, DA (ed.) 2003, 'Absolute optical calibration using a simple tungsten light bulb: Experiment', Proceedings of the 30th Annual European Meeting on Atmospheric Studies by Optical Methods, 1/01/00 pp. 50-54.

APA

Kosch, M. J., Mäkinen, S., Sigernes, F., Harang, O., Sigernes, F. (Ed.), & Lorentzen, D. A. (Ed.) (2003). Absolute optical calibration using a simple tungsten light bulb: Experiment. 50-54. Proceedings of the 30th Annual European Meeting on Atmospheric Studies by Optical Methods.

Vancouver

Kosch MJ, Mäkinen S, Sigernes F, Harang O, Sigernes F, (ed.), Lorentzen DA, (ed.). Absolute optical calibration using a simple tungsten light bulb: Experiment. 2003. Proceedings of the 30th Annual European Meeting on Atmospheric Studies by Optical Methods.

Author

Kosch, M. J. ; Mäkinen, S. ; Sigernes, F. et al. / Absolute optical calibration using a simple tungsten light bulb: Experiment. Proceedings of the 30th Annual European Meeting on Atmospheric Studies by Optical Methods.5 p.

Bibtex

@conference{a7a6586d79524c2b9edaad3d3645e130,
title = "Absolute optical calibration using a simple tungsten light bulb: Experiment",
abstract = "Absolute spectral intensity calibration of optical detectors has always been difficult. Up to now it was only possible through the use of expensive sources, which are cross-calibrated against national standards. At the 28AM optical meeting, a simple theoretical approach to absolute optical calibrations was described using any ordinary tungsten light bulb [1]. A key element of the theory is transforming tungsten into its equivalent blackbody radiator. This permits direct application of Stefan-Bolzmann{\textquoteright}s and Planck{\textquoteright}s formulas of radiation. The theory has been tested by comparing three household tungsten light bulbs with a calibrated source at several wavelengths typically used in auroral research. The results of this experiment are most encouraging.",
keywords = "DCS-publications-id, inproc-326, DCS-publications-credits, iono-fa, DCS-publications-personnel-id, 7",
author = "Kosch, {M. J.} and S. M{\"a}kinen and F. Sigernes and O. Harang and F. Sigernes and Lorentzen, {D. A.}",
year = "2003",
language = "English",
pages = "50--54",
note = "Proceedings of the 30th Annual European Meeting on Atmospheric Studies by Optical Methods ; Conference date: 01-01-1900",

}

RIS

TY - CONF

T1 - Absolute optical calibration using a simple tungsten light bulb: Experiment

AU - Kosch, M. J.

AU - Mäkinen, S.

AU - Sigernes, F.

AU - Harang, O.

A2 - Sigernes, F.

A2 - Lorentzen, D. A.

PY - 2003

Y1 - 2003

N2 - Absolute spectral intensity calibration of optical detectors has always been difficult. Up to now it was only possible through the use of expensive sources, which are cross-calibrated against national standards. At the 28AM optical meeting, a simple theoretical approach to absolute optical calibrations was described using any ordinary tungsten light bulb [1]. A key element of the theory is transforming tungsten into its equivalent blackbody radiator. This permits direct application of Stefan-Bolzmann’s and Planck’s formulas of radiation. The theory has been tested by comparing three household tungsten light bulbs with a calibrated source at several wavelengths typically used in auroral research. The results of this experiment are most encouraging.

AB - Absolute spectral intensity calibration of optical detectors has always been difficult. Up to now it was only possible through the use of expensive sources, which are cross-calibrated against national standards. At the 28AM optical meeting, a simple theoretical approach to absolute optical calibrations was described using any ordinary tungsten light bulb [1]. A key element of the theory is transforming tungsten into its equivalent blackbody radiator. This permits direct application of Stefan-Bolzmann’s and Planck’s formulas of radiation. The theory has been tested by comparing three household tungsten light bulbs with a calibrated source at several wavelengths typically used in auroral research. The results of this experiment are most encouraging.

KW - DCS-publications-id

KW - inproc-326

KW - DCS-publications-credits

KW - iono-fa

KW - DCS-publications-personnel-id

KW - 7

M3 - Other

SP - 50

EP - 54

T2 - Proceedings of the 30th Annual European Meeting on Atmospheric Studies by Optical Methods

Y2 - 1 January 1900

ER -