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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/marciana/2004/01.08.13.56   (restricted access)
Last Update2009:03.11.18.11.21 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/01.08.13.56.39
Metadata Last Update2018:06.05.01.20.41 (UTC) administrator
Secondary KeyINPE-10377-PRE/5877
Citation KeySantosLewi:2003:ShWaSt
TitleShock Wave Structure in a Rarefied Hypersonic Flow on Power Law Shaped Leading Edges
FormatOn-line
Year2003
Access Date2024, Apr. 27
Secondary TypePRE CI
Number of Files1
Size437 KiB
2. Context
Author1 Santos, Wilson Fernando Nogueira
2 Lewis, Mark J.
Group1 LCP-INPE-MCT-BR
Affiliation1 Combustion and Propulsion Laboratory
2 National Institute for Space Research
Conference NameAIAA Aerospace Sciences Meeting and Exhibit, 41.
Conference LocationReno, NV
Date6-9, 2003
PublisherAIAA
Publisher CityReston, VA
Pages1-11
Book TitleProceedings
History (UTC)2008-06-10 23:02:09 :: administrator -> marciana ::
2009-03-11 18:11:21 :: marciana -> administrator ::
2018-06-05 01:20:41 :: administrator -> marciana :: 2003
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordspropulsão
power law
shaped leading edges
hypersonic flow
Direct Simulation Monte Carlo method
DSMC
AbstractThis work deals with a numerical study on power law shaped leading edges situated in a rarefied hypersonic flow. The work is motivated by interest in investigating the flowfield structure of power-law shaped leading edges as possible candidates for blunting geometries of hypersonic leading edges. The primary aim of this paper is to examine in details the geometry effect of such leading edges on the shock wave structure. The sensitivity of the shock wave shape, standoff distance and shock wave thickness to shape variations of such leading edges is calculated by using a Direct Simulation Monte Carlo method. Calculations show that the shock wave shape is in surprising agreement with that predicted by the hypersonic small disturbance theory for the flow conditions considered.
AreaCOMB
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > LABCP > Shock Wave Structure...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Fileshock.pdf
User Groupadministrator
marciana
Visibilityshown
Copy HolderSID/SCD
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ET38CH
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Notes(AIAA 2003/1134)
Empty Fieldsarchivingpolicy archivist callnumber copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress identifier isbn issn label lineage mark mirrorrepository nextedition numberofvolumes orcid organization parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume
7. Description control
e-Mail (login)marciana
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