A new flux splitting scheme
A new flux splitting scheme is proposed. The scheme is remarkably simple and yet its accuracy rivals and in some cases surpasses that of Roe's solver in the Euler and Navier-Stokes solutions performed in this study. The scheme is robust and converges as fast as the Roe splitting. An approximate...
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creator | Liou, Meng-Sing Steffen, Christopher J., Jr |
description | A new flux splitting scheme is proposed. The scheme is remarkably simple and yet its accuracy rivals and in some cases surpasses that of Roe's solver in the Euler and Navier-Stokes solutions performed in this study. The scheme is robust and converges as fast as the Roe splitting. An approximately defined cell-face advection Mach number is proposed using values from the two straddling cells via associated characteristic speeds. This interface Mach number is then used to determine the upwind extrapolation for the convective quantities. Accordingly, the name of the scheme is coined as Advection Upstream Splitting Method (AUSM). A new pressure splitting is introduced which is shown to behave successfully, yielding much smoother results than other existing pressure splittings. Of particular interest is the supersonic blunt body problem in which the Roe scheme gives anomalous solutions. The AUSM produces correct solutions without difficulty for a wide range of flow conditions as well as grids. |
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The scheme is remarkably simple and yet its accuracy rivals and in some cases surpasses that of Roe's solver in the Euler and Navier-Stokes solutions performed in this study. The scheme is robust and converges as fast as the Roe splitting. An approximately defined cell-face advection Mach number is proposed using values from the two straddling cells via associated characteristic speeds. This interface Mach number is then used to determine the upwind extrapolation for the convective quantities. Accordingly, the name of the scheme is coined as Advection Upstream Splitting Method (AUSM). A new pressure splitting is introduced which is shown to behave successfully, yielding much smoother results than other existing pressure splittings. Of particular interest is the supersonic blunt body problem in which the Roe scheme gives anomalous solutions. The AUSM produces correct solutions without difficulty for a wide range of flow conditions as well as grids.</description><language>eng</language><publisher>Legacy CDMS</publisher><subject>Numerical Analysis</subject><creationdate>1991</creationdate><rights>Copyright Determination: GOV_PUBLIC_USE_PERMITTED</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>778,798</link.rule.ids><linktorsrc>$$Uhttps://ntrs.nasa.gov/citations/19910013501$$EView_record_in_NASA$$FView_record_in_$$GNASA$$Hfree_for_read</linktorsrc></links><search><creatorcontrib>Liou, Meng-Sing</creatorcontrib><creatorcontrib>Steffen, Christopher J., Jr</creatorcontrib><title>A new flux splitting scheme</title><description>A new flux splitting scheme is proposed. The scheme is remarkably simple and yet its accuracy rivals and in some cases surpasses that of Roe's solver in the Euler and Navier-Stokes solutions performed in this study. The scheme is robust and converges as fast as the Roe splitting. An approximately defined cell-face advection Mach number is proposed using values from the two straddling cells via associated characteristic speeds. This interface Mach number is then used to determine the upwind extrapolation for the convective quantities. Accordingly, the name of the scheme is coined as Advection Upstream Splitting Method (AUSM). A new pressure splitting is introduced which is shown to behave successfully, yielding much smoother results than other existing pressure splittings. Of particular interest is the supersonic blunt body problem in which the Roe scheme gives anomalous solutions. The AUSM produces correct solutions without difficulty for a wide range of flow conditions as well as grids.</description><subject>Numerical Analysis</subject><fulltext>true</fulltext><rsrctype>report</rsrctype><creationdate>1991</creationdate><recordtype>report</recordtype><sourceid>CYI</sourceid><recordid>eNrjZJB2VMhLLVdIyymtUCguyMksKcnMS1coTs5IzU3lYWBNS8wpTuWF0twMMm6uIc4eunmJxYnxeSVFxfGGlpaGBgaGxqZATEAaANwUHwk</recordid><startdate>19910501</startdate><enddate>19910501</enddate><creator>Liou, Meng-Sing</creator><creator>Steffen, Christopher J., Jr</creator><scope>CYE</scope><scope>CYI</scope></search><sort><creationdate>19910501</creationdate><title>A new flux splitting scheme</title><author>Liou, Meng-Sing ; Steffen, Christopher J., Jr</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-nasa_ntrs_199100135013</frbrgroupid><rsrctype>reports</rsrctype><prefilter>reports</prefilter><language>eng</language><creationdate>1991</creationdate><topic>Numerical Analysis</topic><toplevel>online_resources</toplevel><creatorcontrib>Liou, Meng-Sing</creatorcontrib><creatorcontrib>Steffen, Christopher J., Jr</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Liou, Meng-Sing</au><au>Steffen, Christopher J., Jr</au><format>book</format><genre>unknown</genre><ristype>RPRT</ristype><btitle>A new flux splitting scheme</btitle><date>1991-05-01</date><risdate>1991</risdate><abstract>A new flux splitting scheme is proposed. The scheme is remarkably simple and yet its accuracy rivals and in some cases surpasses that of Roe's solver in the Euler and Navier-Stokes solutions performed in this study. The scheme is robust and converges as fast as the Roe splitting. An approximately defined cell-face advection Mach number is proposed using values from the two straddling cells via associated characteristic speeds. This interface Mach number is then used to determine the upwind extrapolation for the convective quantities. Accordingly, the name of the scheme is coined as Advection Upstream Splitting Method (AUSM). A new pressure splitting is introduced which is shown to behave successfully, yielding much smoother results than other existing pressure splittings. Of particular interest is the supersonic blunt body problem in which the Roe scheme gives anomalous solutions. The AUSM produces correct solutions without difficulty for a wide range of flow conditions as well as grids.</abstract><cop>Legacy CDMS</cop><oa>free_for_read</oa></addata></record> |
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title | A new flux splitting scheme |
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