Please use this identifier to cite or link to this item: http://repository.futminna.edu.ng:8080/jspui/handle/123456789/896
Title: Optical Path Length, Temperature, and Wavelength Effects Simulation on Ozone Gas Absorption Cross Sections towards Green Communications
Authors: David, Michael
Ibrahim, Mohd Haniff
Idrus, Sevia Mahdaliza
Ngajikin, Nor Hafizah
Azmi, Asrul Izam
En Marcus, Tay Ching
Keywords: Absorption cross sections, length, ozone, pressure, transmittance, visible spectrum
Issue Date: 3-Sep-2016
Publisher: JOURNAL OF ELECTRONIC SCIENCE AND TECHNOLOGY
Abstract: Ozone is a green house gas. Ozone absorption cross sections have been reported with discrepancies and inconsistencies. In this paper, simultaneous effects of the optical path length and temperature variations on ozone gas absorption cross sections are investigated at different wavelengths. HITRAN 2012, the latest available line list on spectralcalc.com simulator, is used in this study to simulate ozone gas absorption cross sections in relation to the simultaneous effects ofthe optical path length and temperature at the wavelengths of 603 nm and 575nm. Results obtained for gas cells with the optical path length from 10cm to 120cm show that the decrease in temperatures from 313 K to 103K results in the increase in ozone gas absorption cross sections. At wavelengths of 603 nm and 575nm, the percentage increase of ozone gas absorption cross sections is 1.22% and 0.71%, respectively. Results obtained in this study show that in the visible spectrum, at constant pressure, ozone gas absorption cross sections are dependent on the temperature and wavelength but do not depend on the optical path length. Analysis in this work addresses discrepancies in ozone gas absorption cross sections in relation to the temperature in the visible spectrum; thus, the results can be applied to get optimal configuration of high accuracy ozone gas sensors.
URI: http://repository.futminna.edu.ng:8080/jspui/handle/123456789/896
Appears in Collections:Telecommunication Engineering

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