Optical analysis of the liquid layer combustion of paraffin-based hybrid rocket fuels
Liquefying hybrid rocket fuels (e.g. paraffin) enable higher regression rates due to the presence of an unstable melt layer on the fuel surface during combustion, which causes entrainment of liquid droplets into the oxidizer gas flow. In order to better understand the mechanism responsible for the d...
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description | Liquefying hybrid rocket fuels (e.g. paraffin) enable higher regression rates due to the presence of an unstable melt layer on the fuel surface during combustion, which causes entrainment of liquid droplets into the oxidizer gas flow. In order to better understand the mechanism responsible for the droplets entrainment, the combustion behaviour of paraffin-based hybrid rocket fuels in combination with gaseous oxygen (GOX) was investigated in the framework of this research. Tests were performed in a 2D slab burner configuration at atmospheric conditions. High-speed videos were recorded and analysed with two different decomposition techniques, applied to the scalar field of the flame luminosity (the flame front is assumed to follow the liquid layer). The fuel slab composition and configuration and the oxidizer mass flow have been varied in order to study the influence of these parameters on the liquid layer instability process. The main focus of the research is to understand the relation between the unstable waves which enable the droplets entrainment process and the regression rate. The results show that the combustion is dominated by periodic, wave-like structures for all the analysed fuels. The frequencies and the wavelengths characterizing the liquid melt layer depend on the fuel viscosity and geometry and on the oxidizer mass flow. Moreover, a dependency of the regression rate on the most excited frequencies and longitudinal wavelengths was found. This is important to better understand the relation between the increased regression rate and the onset and development of the entrainment process, which is connected to the amplification of longitudinal unstable waves caused by the high velocity gas flow over the fuel surface.
•Frequencies and wavelengths of the melt layer depend on the fuel geometry.•Frequencies and wavelengths of the melt layer depend on the fuel viscosity.•Frequencies and wavelengths of the melt layer depend on the oxidizer mass flux.•Unstable waves of the fuel melt layer and Regression rate are correlated.•Kelvin-Helmholtz instability studied under real combustion conditions. |
doi_str_mv | 10.1016/j.actaastro.2018.05.059 |
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•Frequencies and wavelengths of the melt layer depend on the fuel geometry.•Frequencies and wavelengths of the melt layer depend on the fuel viscosity.•Frequencies and wavelengths of the melt layer depend on the oxidizer mass flux.•Unstable waves of the fuel melt layer and Regression rate are correlated.•Kelvin-Helmholtz instability studied under real combustion conditions.</description><identifier>ISSN: 0094-5765</identifier><identifier>EISSN: 1879-2030</identifier><identifier>DOI: 10.1016/j.actaastro.2018.05.059</identifier><language>eng</language><publisher>Elmsford: Elsevier Ltd</publisher><subject>Combustion ; Configurations ; Dependence ; Droplets ; Entrainment ; Flame propagation ; Fuels ; Gas flow ; Hybrid rocket propulsion ; Independent component analysis ; Instability ; Kelvin-Helmholtz instability ; Liquefaction ; Luminosity ; Mass flow ; Optical analysis ; Optical investigations ; Oxygen ; Paraffin-based fuels ; Paraffins ; Proper orthogonal decomposition ; Regression analysis ; Rocket propellants ; Rockets ; Stability ; Viscosity ; Wavelengths</subject><ispartof>Acta astronautica, 2019-05, Vol.158, p.313-322</ispartof><rights>2018 IAA</rights><rights>Copyright Elsevier BV May 2019</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c343t-64823c0824e1bb29b60110ed319a5ba7eb1b486a6ab4c54d1654594af4413d073</citedby><cites>FETCH-LOGICAL-c343t-64823c0824e1bb29b60110ed319a5ba7eb1b486a6ab4c54d1654594af4413d073</cites><orcidid>0000-0002-3714-9664 ; 0000-0002-1708-3944</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/j.actaastro.2018.05.059$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,780,784,3550,27924,27925,45995</link.rule.ids></links><search><creatorcontrib>Petrarolo, Anna</creatorcontrib><creatorcontrib>Kobald, Mario</creatorcontrib><creatorcontrib>Schlechtriem, Stefan</creatorcontrib><title>Optical analysis of the liquid layer combustion of paraffin-based hybrid rocket fuels</title><title>Acta astronautica</title><description>Liquefying hybrid rocket fuels (e.g. paraffin) enable higher regression rates due to the presence of an unstable melt layer on the fuel surface during combustion, which causes entrainment of liquid droplets into the oxidizer gas flow. In order to better understand the mechanism responsible for the droplets entrainment, the combustion behaviour of paraffin-based hybrid rocket fuels in combination with gaseous oxygen (GOX) was investigated in the framework of this research. Tests were performed in a 2D slab burner configuration at atmospheric conditions. High-speed videos were recorded and analysed with two different decomposition techniques, applied to the scalar field of the flame luminosity (the flame front is assumed to follow the liquid layer). The fuel slab composition and configuration and the oxidizer mass flow have been varied in order to study the influence of these parameters on the liquid layer instability process. The main focus of the research is to understand the relation between the unstable waves which enable the droplets entrainment process and the regression rate. The results show that the combustion is dominated by periodic, wave-like structures for all the analysed fuels. The frequencies and the wavelengths characterizing the liquid melt layer depend on the fuel viscosity and geometry and on the oxidizer mass flow. Moreover, a dependency of the regression rate on the most excited frequencies and longitudinal wavelengths was found. This is important to better understand the relation between the increased regression rate and the onset and development of the entrainment process, which is connected to the amplification of longitudinal unstable waves caused by the high velocity gas flow over the fuel surface.
•Frequencies and wavelengths of the melt layer depend on the fuel geometry.•Frequencies and wavelengths of the melt layer depend on the fuel viscosity.•Frequencies and wavelengths of the melt layer depend on the oxidizer mass flux.•Unstable waves of the fuel melt layer and Regression rate are correlated.•Kelvin-Helmholtz instability studied under real combustion conditions.</description><subject>Combustion</subject><subject>Configurations</subject><subject>Dependence</subject><subject>Droplets</subject><subject>Entrainment</subject><subject>Flame propagation</subject><subject>Fuels</subject><subject>Gas flow</subject><subject>Hybrid rocket propulsion</subject><subject>Independent component analysis</subject><subject>Instability</subject><subject>Kelvin-Helmholtz instability</subject><subject>Liquefaction</subject><subject>Luminosity</subject><subject>Mass flow</subject><subject>Optical analysis</subject><subject>Optical investigations</subject><subject>Oxygen</subject><subject>Paraffin-based fuels</subject><subject>Paraffins</subject><subject>Proper orthogonal decomposition</subject><subject>Regression analysis</subject><subject>Rocket propellants</subject><subject>Rockets</subject><subject>Stability</subject><subject>Viscosity</subject><subject>Wavelengths</subject><issn>0094-5765</issn><issn>1879-2030</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNqFkEtrwzAQhEVpoWna31BBz05XtvzQMYS-IJBLcxYrWSZyHcuR5IL_fR1Sei0M7GG_GZgh5JHBigErntsV6ogYonerFFi1gnyWuCILVpUiSSGDa7IAEDzJyyK_JXchtABQppVYkP1uiFZjR7HHbgo2UNfQeDC0s6fR1rTDyXiq3VGNIVrXn98Demwa2ycKg6npYVJ-Jr3TXybSZjRduCc3DXbBPPzeJdm_vnxu3pPt7u1js94mOuNZTApepZmGKuWGKZUKVQBjYOqMCcwVlkYxxasCC1Rc57xmRc5zwbHhnGU1lNmSPF1yB-9OowlRtm70c5Mg05QVlYCqhJkqL5T2LgRvGjl4e0Q_SQbyvKFs5d-G8ryhhHyWmJ3ri3PuZL6t8TJoa3ptauuNjrJ29t-MH83Jfvk</recordid><startdate>201905</startdate><enddate>201905</enddate><creator>Petrarolo, Anna</creator><creator>Kobald, Mario</creator><creator>Schlechtriem, Stefan</creator><general>Elsevier Ltd</general><general>Elsevier BV</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TB</scope><scope>7TG</scope><scope>8FD</scope><scope>FR3</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-3714-9664</orcidid><orcidid>https://orcid.org/0000-0002-1708-3944</orcidid></search><sort><creationdate>201905</creationdate><title>Optical analysis of the liquid layer combustion of paraffin-based hybrid rocket fuels</title><author>Petrarolo, Anna ; Kobald, Mario ; Schlechtriem, Stefan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c343t-64823c0824e1bb29b60110ed319a5ba7eb1b486a6ab4c54d1654594af4413d073</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Combustion</topic><topic>Configurations</topic><topic>Dependence</topic><topic>Droplets</topic><topic>Entrainment</topic><topic>Flame propagation</topic><topic>Fuels</topic><topic>Gas flow</topic><topic>Hybrid rocket propulsion</topic><topic>Independent component analysis</topic><topic>Instability</topic><topic>Kelvin-Helmholtz instability</topic><topic>Liquefaction</topic><topic>Luminosity</topic><topic>Mass flow</topic><topic>Optical analysis</topic><topic>Optical investigations</topic><topic>Oxygen</topic><topic>Paraffin-based fuels</topic><topic>Paraffins</topic><topic>Proper orthogonal decomposition</topic><topic>Regression analysis</topic><topic>Rocket propellants</topic><topic>Rockets</topic><topic>Stability</topic><topic>Viscosity</topic><topic>Wavelengths</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Petrarolo, Anna</creatorcontrib><creatorcontrib>Kobald, Mario</creatorcontrib><creatorcontrib>Schlechtriem, Stefan</creatorcontrib><collection>CrossRef</collection><collection>Mechanical & Transportation Engineering Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Acta astronautica</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Petrarolo, Anna</au><au>Kobald, Mario</au><au>Schlechtriem, Stefan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Optical analysis of the liquid layer combustion of paraffin-based hybrid rocket fuels</atitle><jtitle>Acta astronautica</jtitle><date>2019-05</date><risdate>2019</risdate><volume>158</volume><spage>313</spage><epage>322</epage><pages>313-322</pages><issn>0094-5765</issn><eissn>1879-2030</eissn><abstract>Liquefying hybrid rocket fuels (e.g. paraffin) enable higher regression rates due to the presence of an unstable melt layer on the fuel surface during combustion, which causes entrainment of liquid droplets into the oxidizer gas flow. In order to better understand the mechanism responsible for the droplets entrainment, the combustion behaviour of paraffin-based hybrid rocket fuels in combination with gaseous oxygen (GOX) was investigated in the framework of this research. Tests were performed in a 2D slab burner configuration at atmospheric conditions. High-speed videos were recorded and analysed with two different decomposition techniques, applied to the scalar field of the flame luminosity (the flame front is assumed to follow the liquid layer). The fuel slab composition and configuration and the oxidizer mass flow have been varied in order to study the influence of these parameters on the liquid layer instability process. The main focus of the research is to understand the relation between the unstable waves which enable the droplets entrainment process and the regression rate. The results show that the combustion is dominated by periodic, wave-like structures for all the analysed fuels. The frequencies and the wavelengths characterizing the liquid melt layer depend on the fuel viscosity and geometry and on the oxidizer mass flow. Moreover, a dependency of the regression rate on the most excited frequencies and longitudinal wavelengths was found. This is important to better understand the relation between the increased regression rate and the onset and development of the entrainment process, which is connected to the amplification of longitudinal unstable waves caused by the high velocity gas flow over the fuel surface.
•Frequencies and wavelengths of the melt layer depend on the fuel geometry.•Frequencies and wavelengths of the melt layer depend on the fuel viscosity.•Frequencies and wavelengths of the melt layer depend on the oxidizer mass flux.•Unstable waves of the fuel melt layer and Regression rate are correlated.•Kelvin-Helmholtz instability studied under real combustion conditions.</abstract><cop>Elmsford</cop><pub>Elsevier Ltd</pub><doi>10.1016/j.actaastro.2018.05.059</doi><tpages>10</tpages><orcidid>https://orcid.org/0000-0002-3714-9664</orcidid><orcidid>https://orcid.org/0000-0002-1708-3944</orcidid></addata></record> |
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subjects | Combustion Configurations Dependence Droplets Entrainment Flame propagation Fuels Gas flow Hybrid rocket propulsion Independent component analysis Instability Kelvin-Helmholtz instability Liquefaction Luminosity Mass flow Optical analysis Optical investigations Oxygen Paraffin-based fuels Paraffins Proper orthogonal decomposition Regression analysis Rocket propellants Rockets Stability Viscosity Wavelengths |
title | Optical analysis of the liquid layer combustion of paraffin-based hybrid rocket fuels |
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