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Lagrangian multi-particle statistics
Combined measurements of the Lagrangian evolution of particle constellations and the coarse-grained velocity derivative tensor ∂ũ i /∂ x j are presented. The data are obtained from three-dimensional particle tracking measurements in a quasi isotropic turbulent flow at an intermediate Reynolds number...
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Published in: | Journal of turbulence 2007-01, Vol.8 (8), p.45-45 |
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creator | Lüthi, Beat Ott, Søren Berg, Jacob Mann, Jakob |
description | Combined measurements of the Lagrangian evolution of particle constellations and the coarse-grained velocity derivative tensor ∂ũ
i
/∂ x
j
are presented. The data are obtained from three-dimensional particle tracking measurements in a quasi isotropic turbulent flow at an intermediate Reynolds number. Particle constellations are followed for as long as one integral time and for several Batchelor times. We suggest a method to obtain ∂ũ
i
/∂ x
j
from velocity measurements at discrete points. Based on an analytical result and on a sensitivity analysis, both presented here, we estimate the accuracy for filtered strain, ᵴ
2
, and enstrophy,
2
, at around 30%. The accuracy improves with higher tracer seeding density and with smaller filter scale Δ. We obtain good scaling with t* = √2r
2
/15S
2
(r) for filtered strain and vorticity and present filtered R-Q invariant maps with the typical 'tear drop' shape that is known from velocity gradients at viscous scales. Lagrangian results are given for the growth of particle pairs, triangles and tetrahedra. Their principal axes are preferentially oriented with the eigenframe of coarse-grained strain, just like constellations with infinitesimal separations are known to do. The compensated separation rate is found to be close to its viscous counterpart as 1/2⟨ (dr
2
/dt)/r
2
⟩· t
*
/√2≈ 0.12. It appears that the contribution from the coarse-grained strain field, r
i
r
j
ᵴ
ij
filtered at scale Δ = r, is responsible for roughly 2/3 of the separation rate, while 1/3 stems from scales Δ < r. |
doi_str_mv | 10.1080/14685240701522927 |
format | article |
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i
/∂ x
j
are presented. The data are obtained from three-dimensional particle tracking measurements in a quasi isotropic turbulent flow at an intermediate Reynolds number. Particle constellations are followed for as long as one integral time and for several Batchelor times. We suggest a method to obtain ∂ũ
i
/∂ x
j
from velocity measurements at discrete points. Based on an analytical result and on a sensitivity analysis, both presented here, we estimate the accuracy for filtered strain, ᵴ
2
, and enstrophy,
2
, at around 30%. The accuracy improves with higher tracer seeding density and with smaller filter scale Δ. We obtain good scaling with t* = √2r
2
/15S
2
(r) for filtered strain and vorticity and present filtered R-Q invariant maps with the typical 'tear drop' shape that is known from velocity gradients at viscous scales. Lagrangian results are given for the growth of particle pairs, triangles and tetrahedra. Their principal axes are preferentially oriented with the eigenframe of coarse-grained strain, just like constellations with infinitesimal separations are known to do. The compensated separation rate is found to be close to its viscous counterpart as 1/2⟨ (dr
2
/dt)/r
2
⟩· t
*
/√2≈ 0.12. It appears that the contribution from the coarse-grained strain field, r
i
r
j
ᵴ
ij
filtered at scale Δ = r, is responsible for roughly 2/3 of the separation rate, while 1/3 stems from scales Δ < r.</description><identifier>ISSN: 1468-5248</identifier><identifier>EISSN: 1468-5248</identifier><identifier>DOI: 10.1080/14685240701522927</identifier><language>eng</language><publisher>Taylor & Francis Group</publisher><subject>Lagrangian evolution ; Multi-particle statistics ; Particle tracking ; Velocity gradient</subject><ispartof>Journal of turbulence, 2007-01, Vol.8 (8), p.45-45</ispartof><rights>Copyright Taylor & Francis Group, LLC 2007</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c408t-b8a757cc0041cee56a9d3aba6a1da67cc0cbbf86cdd4f758e5d18d82abfec58e3</citedby><cites>FETCH-LOGICAL-c408t-b8a757cc0041cee56a9d3aba6a1da67cc0cbbf86cdd4f758e5d18d82abfec58e3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Lüthi, Beat</creatorcontrib><creatorcontrib>Ott, Søren</creatorcontrib><creatorcontrib>Berg, Jacob</creatorcontrib><creatorcontrib>Mann, Jakob</creatorcontrib><title>Lagrangian multi-particle statistics</title><title>Journal of turbulence</title><description>Combined measurements of the Lagrangian evolution of particle constellations and the coarse-grained velocity derivative tensor ∂ũ
i
/∂ x
j
are presented. The data are obtained from three-dimensional particle tracking measurements in a quasi isotropic turbulent flow at an intermediate Reynolds number. Particle constellations are followed for as long as one integral time and for several Batchelor times. We suggest a method to obtain ∂ũ
i
/∂ x
j
from velocity measurements at discrete points. Based on an analytical result and on a sensitivity analysis, both presented here, we estimate the accuracy for filtered strain, ᵴ
2
, and enstrophy,
2
, at around 30%. The accuracy improves with higher tracer seeding density and with smaller filter scale Δ. We obtain good scaling with t* = √2r
2
/15S
2
(r) for filtered strain and vorticity and present filtered R-Q invariant maps with the typical 'tear drop' shape that is known from velocity gradients at viscous scales. Lagrangian results are given for the growth of particle pairs, triangles and tetrahedra. Their principal axes are preferentially oriented with the eigenframe of coarse-grained strain, just like constellations with infinitesimal separations are known to do. The compensated separation rate is found to be close to its viscous counterpart as 1/2⟨ (dr
2
/dt)/r
2
⟩· t
*
/√2≈ 0.12. It appears that the contribution from the coarse-grained strain field, r
i
r
j
ᵴ
ij
filtered at scale Δ = r, is responsible for roughly 2/3 of the separation rate, while 1/3 stems from scales Δ < r.</description><subject>Lagrangian evolution</subject><subject>Multi-particle statistics</subject><subject>Particle tracking</subject><subject>Velocity gradient</subject><issn>1468-5248</issn><issn>1468-5248</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</creationdate><recordtype>article</recordtype><recordid>eNqFkEtLQzEQhYMoWKs_wF0X4u5qkpvXBTdSfEHBja7D3DxK5D5qkqL996bUhVCkq5k5c74ZOAhdEnxDsMK3hAnFKcMSE05pQ-URmmy1qojq-E9_is5S-sCYCMrFBF0tYBlhWAYYZv26y6FaQczBdG6WMuSQSp_O0YmHLrmL3zpF748Pb_PnavH69DK_X1SGYZWrVoHk0hiMGTHOcQGNraEFAcSC2C5M23oljLXMS64ct0RZRaH1zpSxnqLr3d1VHD_XLmXdh2Rc18HgxnXSNWsaWjfyoJGWTJgUrBjJzmjimFJ0Xq9i6CFuNMF6G5zeC64wcseEwY-xh68xdlZn2HRj9CUrE9I-pfN3LuTdQbL-__EP-GeGMA</recordid><startdate>20070101</startdate><enddate>20070101</enddate><creator>Lüthi, Beat</creator><creator>Ott, Søren</creator><creator>Berg, Jacob</creator><creator>Mann, Jakob</creator><general>Taylor & Francis Group</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope><scope>7TB</scope><scope>8FD</scope><scope>FR3</scope><scope>H8D</scope><scope>KR7</scope><scope>L7M</scope></search><sort><creationdate>20070101</creationdate><title>Lagrangian multi-particle statistics</title><author>Lüthi, Beat ; Ott, Søren ; Berg, Jacob ; Mann, Jakob</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c408t-b8a757cc0041cee56a9d3aba6a1da67cc0cbbf86cdd4f758e5d18d82abfec58e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2007</creationdate><topic>Lagrangian evolution</topic><topic>Multi-particle statistics</topic><topic>Particle tracking</topic><topic>Velocity gradient</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Lüthi, Beat</creatorcontrib><creatorcontrib>Ott, Søren</creatorcontrib><creatorcontrib>Berg, Jacob</creatorcontrib><creatorcontrib>Mann, Jakob</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Mechanical & Transportation Engineering Abstracts</collection><collection>Technology Research Database</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Civil Engineering Abstracts</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Journal of turbulence</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Lüthi, Beat</au><au>Ott, Søren</au><au>Berg, Jacob</au><au>Mann, Jakob</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Lagrangian multi-particle statistics</atitle><jtitle>Journal of turbulence</jtitle><date>2007-01-01</date><risdate>2007</risdate><volume>8</volume><issue>8</issue><spage>45</spage><epage>45</epage><pages>45-45</pages><issn>1468-5248</issn><eissn>1468-5248</eissn><abstract>Combined measurements of the Lagrangian evolution of particle constellations and the coarse-grained velocity derivative tensor ∂ũ
i
/∂ x
j
are presented. The data are obtained from three-dimensional particle tracking measurements in a quasi isotropic turbulent flow at an intermediate Reynolds number. Particle constellations are followed for as long as one integral time and for several Batchelor times. We suggest a method to obtain ∂ũ
i
/∂ x
j
from velocity measurements at discrete points. Based on an analytical result and on a sensitivity analysis, both presented here, we estimate the accuracy for filtered strain, ᵴ
2
, and enstrophy,
2
, at around 30%. The accuracy improves with higher tracer seeding density and with smaller filter scale Δ. We obtain good scaling with t* = √2r
2
/15S
2
(r) for filtered strain and vorticity and present filtered R-Q invariant maps with the typical 'tear drop' shape that is known from velocity gradients at viscous scales. Lagrangian results are given for the growth of particle pairs, triangles and tetrahedra. Their principal axes are preferentially oriented with the eigenframe of coarse-grained strain, just like constellations with infinitesimal separations are known to do. The compensated separation rate is found to be close to its viscous counterpart as 1/2⟨ (dr
2
/dt)/r
2
⟩· t
*
/√2≈ 0.12. It appears that the contribution from the coarse-grained strain field, r
i
r
j
ᵴ
ij
filtered at scale Δ = r, is responsible for roughly 2/3 of the separation rate, while 1/3 stems from scales Δ < r.</abstract><pub>Taylor & Francis Group</pub><doi>10.1080/14685240701522927</doi><tpages>1</tpages></addata></record> |
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language | eng |
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source | Taylor and Francis Science and Technology Collection |
subjects | Lagrangian evolution Multi-particle statistics Particle tracking Velocity gradient |
title | Lagrangian multi-particle statistics |
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