IR microcavity light emitters for gas detection

E. Hadji; E. Picard; C. Roux; P. Ferret; P. Ferret; E. Molva

Conference on Lasers and Electro-Optics
OSA Technical Digest (Optica Publishing Group, 2000),
paper CMA2

IR microcavity light emitters for gas detection

E. Hadji, E. Picard, C. Roux, P. Ferret, and E. Molva

Conference on Lasers and Electro-Optics 2000

San Francisco, California United States
7–11 May 2000
ISBN: 1-55752-634-6

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Novel Semiconductor Structures (CMA)

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E. Hadji, E. Picard, C. Roux, P. Ferret, and E. Molva, "IR microcavity light emitters for gas detection," in Conference on Lasers and Electro-Optics, S. Brueck, R. Fields, M. Fejer, and F. Leonberger, eds., OSA Technical Digest (Optica Publishing Group, 2000), paper CMA2.

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Abstract

Optical gas monitoring would require light sources above 3 µm because most of the gas species (CO, CO₂, NO_x, HCl, SO₂, N₂O, NH₃., CH₄ …) have their fundamental absorption lines between 3 and 6 µ.m.

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