Analysis of Expected Skin Burns from Accepted Process Flare Heat Radiation Levels to Public Passersby

Hot flaring, even from quite high flare stacks, may result in significant heat radiation outside a facility to, e.g., public roads where random passersby may be exposed. The present study suggests a novel method for analyzing a typical flare heat radiation exposure and investigates skin burns that m...

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Main Author: Torgrim Log
Format: Article
Language:English
Published: MDPI AG 2021-09-01
Series:Energies
Subjects:
Online Access:https://www.mdpi.com/1996-1073/14/17/5474
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spelling doaj-158acfb5484b40ef854188c9ba0a12a62021-09-09T13:43:39ZengMDPI AGEnergies1996-10732021-09-01145474547410.3390/en14175474Analysis of Expected Skin Burns from Accepted Process Flare Heat Radiation Levels to Public PassersbyTorgrim Log0Chemistry and Biomedical Laboratory Sciences, Fire Disasters Research Group, Department of Safety, Western Norway University of Applied Sciences, 5528 Haugesund, NorwayHot flaring, even from quite high flare stacks, may result in significant heat radiation outside a facility to, e.g., public roads where random passersby may be exposed. The present study suggests a novel method for analyzing a typical flare heat radiation exposure and investigates skin burns that may be inflicted on an exposed person if a facility needs to depressurize in an emergency situation. A typical radiation field from an ignited natural gas vent was taken as the boundary condition, and these values were compared to radiation levels mentioned by the American Petroleum Institute (API 521), e.g., 1.58 kW/m<sup>2</sup> and above. Due to facility perimeter fences along roads in larger industry areas, it was assumed that an exposed person may flee along a road rather than in the ideal direction away from the flare. It was assumed that naked skin, e.g., a bare shoulder or a bald head is exposed. The Pennes bioheat equation was numerically solved for the skin layers while the person escapes along the road. Sun radiation and convective heat exchange to the ambient air were included, and the subsequent skin injury was calculated based on the temperature development in the basal layer. Parameters affecting burn severity, such as heat radiation, solar radiation, and convective heat transfer coefficient, were analyzed. For small flares and ignited small cold vents, no skin burn would be expected for 1.58 kW/m<sup>2</sup> or 3.16 kW/m<sup>2</sup> maximum heat radiation at the skin surface. However, higher flare rates corresponding to, e.g., 4.0 kW/m<sup>2</sup> maximum flare heat radiation to the skin, resulted both in higher basal layer temperatures and longer exposure time, thus increasing the damage integral significantly. It is demonstrated that the novel approach works well. In future studies, it may, e.g., be extended to cover escape through partly shielded escape routes.https://www.mdpi.com/1996-1073/14/17/5474natural gas flaringpassersbyradiant heat exposureskin burnsmodeling
collection DOAJ
language English
format Article
sources DOAJ
author Torgrim Log
spellingShingle Torgrim Log
Analysis of Expected Skin Burns from Accepted Process Flare Heat Radiation Levels to Public Passersby
Energies
natural gas flaring
passersby
radiant heat exposure
skin burns
modeling
author_facet Torgrim Log
author_sort Torgrim Log
title Analysis of Expected Skin Burns from Accepted Process Flare Heat Radiation Levels to Public Passersby
title_short Analysis of Expected Skin Burns from Accepted Process Flare Heat Radiation Levels to Public Passersby
title_full Analysis of Expected Skin Burns from Accepted Process Flare Heat Radiation Levels to Public Passersby
title_fullStr Analysis of Expected Skin Burns from Accepted Process Flare Heat Radiation Levels to Public Passersby
title_full_unstemmed Analysis of Expected Skin Burns from Accepted Process Flare Heat Radiation Levels to Public Passersby
title_sort analysis of expected skin burns from accepted process flare heat radiation levels to public passersby
publisher MDPI AG
series Energies
issn 1996-1073
publishDate 2021-09-01
description Hot flaring, even from quite high flare stacks, may result in significant heat radiation outside a facility to, e.g., public roads where random passersby may be exposed. The present study suggests a novel method for analyzing a typical flare heat radiation exposure and investigates skin burns that may be inflicted on an exposed person if a facility needs to depressurize in an emergency situation. A typical radiation field from an ignited natural gas vent was taken as the boundary condition, and these values were compared to radiation levels mentioned by the American Petroleum Institute (API 521), e.g., 1.58 kW/m<sup>2</sup> and above. Due to facility perimeter fences along roads in larger industry areas, it was assumed that an exposed person may flee along a road rather than in the ideal direction away from the flare. It was assumed that naked skin, e.g., a bare shoulder or a bald head is exposed. The Pennes bioheat equation was numerically solved for the skin layers while the person escapes along the road. Sun radiation and convective heat exchange to the ambient air were included, and the subsequent skin injury was calculated based on the temperature development in the basal layer. Parameters affecting burn severity, such as heat radiation, solar radiation, and convective heat transfer coefficient, were analyzed. For small flares and ignited small cold vents, no skin burn would be expected for 1.58 kW/m<sup>2</sup> or 3.16 kW/m<sup>2</sup> maximum heat radiation at the skin surface. However, higher flare rates corresponding to, e.g., 4.0 kW/m<sup>2</sup> maximum flare heat radiation to the skin, resulted both in higher basal layer temperatures and longer exposure time, thus increasing the damage integral significantly. It is demonstrated that the novel approach works well. In future studies, it may, e.g., be extended to cover escape through partly shielded escape routes.
topic natural gas flaring
passersby
radiant heat exposure
skin burns
modeling
url https://www.mdpi.com/1996-1073/14/17/5474
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