Compressible Flow Phenomena at Inception of Lateral Density Currents Fed by Collapsing Gas‐Particle Mixtures
Many geological flows are sourced by falling gas‐particle mixtures, such as during collapse of lava domes, and impulsive eruptive jets, and sustained columns, and rock falls. The transition from vertical to lateral flow is complex due to the range of coupling between particles of different sizes and...
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Veröffentlicht in: | Journal of geophysical research. Solid earth 2018-02, Vol.123 (2), p.1286-1302 |
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description | Many geological flows are sourced by falling gas‐particle mixtures, such as during collapse of lava domes, and impulsive eruptive jets, and sustained columns, and rock falls. The transition from vertical to lateral flow is complex due to the range of coupling between particles of different sizes and densities and the carrier gas, and due to the potential for compressible flow phenomena. We use multiphase modeling to explore these dynamics. In mixtures with small particles, and with subsonic speeds, particles follow the gas such that outgoing lateral flows have similar particle concentration and speed as the vertical flows. Large particles concentrate immediately upon impact and move laterally away as granular flows overridden by a high‐speed jet of expelled gas. When a falling flow is supersonic, a bow shock develops above the impact zone, and this produces a zone of high pressure from which lateral flows emerge as overpressured wall jets. The jets form complex structures as the mixtures expand and accelerate and then recompress through a recompression zone that mimics a Mach disk shock in ideal gas jets. In mixtures with moderate to high ratios of fine to coarse particles, the latter tend to follow fine particles through the expansion‐recompression flow fields because of particle‐particle drag. Expansion within the flow fields can lead to locally reduced gas pressure that could enhance substrate erosion in natural flows. The recompression zones form at distances, and have peak pressures, that are roughly proportional to the Mach numbers of impacting flows.
Key Points
Dynamics of geological flows fed by collapsing mixtures strongly depends upon particle‐gas coupling
Fine particles can reduce sound speed in the collapsing mixtures, resulting in additional compressible flow phenomena in proximal lateral flows
Polydisperse cases exhibit hybrid behavior determined by both particle‐gas coupling and Mach number, depending upon relative proportions of particle sizes |
doi_str_mv | 10.1002/2017JB015129 |
format | Article |
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Key Points
Dynamics of geological flows fed by collapsing mixtures strongly depends upon particle‐gas coupling
Fine particles can reduce sound speed in the collapsing mixtures, resulting in additional compressible flow phenomena in proximal lateral flows
Polydisperse cases exhibit hybrid behavior determined by both particle‐gas coupling and Mach number, depending upon relative proportions of particle sizes</description><identifier>ISSN: 2169-9313</identifier><identifier>EISSN: 2169-9356</identifier><identifier>DOI: 10.1002/2017JB015129</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Carrier density ; Columns (structural) ; Compressible flow ; Compressing ; Density currents ; Dynamics ; Erosion ; Falling ; Fields ; Flow ; Gas jets ; Gas pressure ; Geophysics ; High pressure ; Ideal gas ; impinging jet ; Jets ; Lava ; Lava domes ; Mach number ; Modelling ; multiphase flow ; Particle concentration ; Pressure ; pyroclastic density current ; Ratios ; Rock falls ; Stokes number ; Substrates ; Wall jets</subject><ispartof>Journal of geophysical research. Solid earth, 2018-02, Vol.123 (2), p.1286-1302</ispartof><rights>2018. American Geophysical Union. All Rights Reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a3961-ba2abe55437e3c432f19e32d5e90ea333ab8a509dab84e7c539640c9855eed0a3</citedby><cites>FETCH-LOGICAL-a3961-ba2abe55437e3c432f19e32d5e90ea333ab8a509dab84e7c539640c9855eed0a3</cites><orcidid>0000-0002-8133-5878</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1002%2F2017JB015129$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1002%2F2017JB015129$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,1411,1427,27903,27904,45553,45554,46387,46811</link.rule.ids></links><search><creatorcontrib>Valentine, Greg A.</creatorcontrib><creatorcontrib>Sweeney, Matthew R.</creatorcontrib><title>Compressible Flow Phenomena at Inception of Lateral Density Currents Fed by Collapsing Gas‐Particle Mixtures</title><title>Journal of geophysical research. Solid earth</title><description>Many geological flows are sourced by falling gas‐particle mixtures, such as during collapse of lava domes, and impulsive eruptive jets, and sustained columns, and rock falls. The transition from vertical to lateral flow is complex due to the range of coupling between particles of different sizes and densities and the carrier gas, and due to the potential for compressible flow phenomena. We use multiphase modeling to explore these dynamics. In mixtures with small particles, and with subsonic speeds, particles follow the gas such that outgoing lateral flows have similar particle concentration and speed as the vertical flows. Large particles concentrate immediately upon impact and move laterally away as granular flows overridden by a high‐speed jet of expelled gas. When a falling flow is supersonic, a bow shock develops above the impact zone, and this produces a zone of high pressure from which lateral flows emerge as overpressured wall jets. The jets form complex structures as the mixtures expand and accelerate and then recompress through a recompression zone that mimics a Mach disk shock in ideal gas jets. In mixtures with moderate to high ratios of fine to coarse particles, the latter tend to follow fine particles through the expansion‐recompression flow fields because of particle‐particle drag. Expansion within the flow fields can lead to locally reduced gas pressure that could enhance substrate erosion in natural flows. The recompression zones form at distances, and have peak pressures, that are roughly proportional to the Mach numbers of impacting flows.
Key Points
Dynamics of geological flows fed by collapsing mixtures strongly depends upon particle‐gas coupling
Fine particles can reduce sound speed in the collapsing mixtures, resulting in additional compressible flow phenomena in proximal lateral flows
Polydisperse cases exhibit hybrid behavior determined by both particle‐gas coupling and Mach number, depending upon relative proportions of particle sizes</description><subject>Carrier density</subject><subject>Columns (structural)</subject><subject>Compressible flow</subject><subject>Compressing</subject><subject>Density currents</subject><subject>Dynamics</subject><subject>Erosion</subject><subject>Falling</subject><subject>Fields</subject><subject>Flow</subject><subject>Gas jets</subject><subject>Gas pressure</subject><subject>Geophysics</subject><subject>High pressure</subject><subject>Ideal gas</subject><subject>impinging jet</subject><subject>Jets</subject><subject>Lava</subject><subject>Lava domes</subject><subject>Mach number</subject><subject>Modelling</subject><subject>multiphase flow</subject><subject>Particle concentration</subject><subject>Pressure</subject><subject>pyroclastic density current</subject><subject>Ratios</subject><subject>Rock falls</subject><subject>Stokes number</subject><subject>Substrates</subject><subject>Wall jets</subject><issn>2169-9313</issn><issn>2169-9356</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNp9kE1OwzAQhS0EElXpjgNYYkvAP3ETL2mgpVURFYJ15CQTcJXawU5UuuMInJGTYFSEWDGbNzP6Zp70EDql5IISwi4ZocliQqigTB6gAaNjGUkuxoe_PeXHaOT9moRKw4rGA2Qyu2kdeK-LBvC0sVu8egFjN2AUVh2emxLaTluDbY2XqgOnGnwNxutuh7PeOTCdx1OocBFm2zSq9do845nyn-8fK-U6XYbHd_qt64PNCTqqVeNh9KND9DS9ecxuo-X9bJ5dLSPF5ZhGhWKqACFingAvY85qKoGzSoAkoDjnqkiVILIKGkNSinAVk1KmQgBURPEhOtv_bZ197cF3-dr2zgTL_DunhKZxygJ1vqdKZ713UOet0xvldjkl-Xeo-d9QA873-FY3sPuXzRezh4lgIqb8CwxdeUQ</recordid><startdate>201802</startdate><enddate>201802</enddate><creator>Valentine, Greg A.</creator><creator>Sweeney, Matthew R.</creator><general>Blackwell Publishing Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7ST</scope><scope>7TG</scope><scope>8FD</scope><scope>C1K</scope><scope>F1W</scope><scope>FR3</scope><scope>H8D</scope><scope>H96</scope><scope>KL.</scope><scope>KR7</scope><scope>L.G</scope><scope>L7M</scope><scope>SOI</scope><orcidid>https://orcid.org/0000-0002-8133-5878</orcidid></search><sort><creationdate>201802</creationdate><title>Compressible Flow Phenomena at Inception of Lateral Density Currents Fed by Collapsing Gas‐Particle Mixtures</title><author>Valentine, Greg A. ; Sweeney, Matthew R.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a3961-ba2abe55437e3c432f19e32d5e90ea333ab8a509dab84e7c539640c9855eed0a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Carrier density</topic><topic>Columns (structural)</topic><topic>Compressible flow</topic><topic>Compressing</topic><topic>Density currents</topic><topic>Dynamics</topic><topic>Erosion</topic><topic>Falling</topic><topic>Fields</topic><topic>Flow</topic><topic>Gas jets</topic><topic>Gas pressure</topic><topic>Geophysics</topic><topic>High pressure</topic><topic>Ideal gas</topic><topic>impinging jet</topic><topic>Jets</topic><topic>Lava</topic><topic>Lava domes</topic><topic>Mach number</topic><topic>Modelling</topic><topic>multiphase flow</topic><topic>Particle concentration</topic><topic>Pressure</topic><topic>pyroclastic density current</topic><topic>Ratios</topic><topic>Rock falls</topic><topic>Stokes number</topic><topic>Substrates</topic><topic>Wall jets</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Valentine, Greg A.</creatorcontrib><creatorcontrib>Sweeney, Matthew R.</creatorcontrib><collection>CrossRef</collection><collection>Environment Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Environment Abstracts</collection><jtitle>Journal of geophysical research. Solid earth</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Valentine, Greg A.</au><au>Sweeney, Matthew R.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Compressible Flow Phenomena at Inception of Lateral Density Currents Fed by Collapsing Gas‐Particle Mixtures</atitle><jtitle>Journal of geophysical research. Solid earth</jtitle><date>2018-02</date><risdate>2018</risdate><volume>123</volume><issue>2</issue><spage>1286</spage><epage>1302</epage><pages>1286-1302</pages><issn>2169-9313</issn><eissn>2169-9356</eissn><abstract>Many geological flows are sourced by falling gas‐particle mixtures, such as during collapse of lava domes, and impulsive eruptive jets, and sustained columns, and rock falls. The transition from vertical to lateral flow is complex due to the range of coupling between particles of different sizes and densities and the carrier gas, and due to the potential for compressible flow phenomena. We use multiphase modeling to explore these dynamics. In mixtures with small particles, and with subsonic speeds, particles follow the gas such that outgoing lateral flows have similar particle concentration and speed as the vertical flows. Large particles concentrate immediately upon impact and move laterally away as granular flows overridden by a high‐speed jet of expelled gas. When a falling flow is supersonic, a bow shock develops above the impact zone, and this produces a zone of high pressure from which lateral flows emerge as overpressured wall jets. The jets form complex structures as the mixtures expand and accelerate and then recompress through a recompression zone that mimics a Mach disk shock in ideal gas jets. In mixtures with moderate to high ratios of fine to coarse particles, the latter tend to follow fine particles through the expansion‐recompression flow fields because of particle‐particle drag. Expansion within the flow fields can lead to locally reduced gas pressure that could enhance substrate erosion in natural flows. The recompression zones form at distances, and have peak pressures, that are roughly proportional to the Mach numbers of impacting flows.
Key Points
Dynamics of geological flows fed by collapsing mixtures strongly depends upon particle‐gas coupling
Fine particles can reduce sound speed in the collapsing mixtures, resulting in additional compressible flow phenomena in proximal lateral flows
Polydisperse cases exhibit hybrid behavior determined by both particle‐gas coupling and Mach number, depending upon relative proportions of particle sizes</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1002/2017JB015129</doi><tpages>17</tpages><orcidid>https://orcid.org/0000-0002-8133-5878</orcidid></addata></record> |
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subjects | Carrier density Columns (structural) Compressible flow Compressing Density currents Dynamics Erosion Falling Fields Flow Gas jets Gas pressure Geophysics High pressure Ideal gas impinging jet Jets Lava Lava domes Mach number Modelling multiphase flow Particle concentration Pressure pyroclastic density current Ratios Rock falls Stokes number Substrates Wall jets |
title | Compressible Flow Phenomena at Inception of Lateral Density Currents Fed by Collapsing Gas‐Particle Mixtures |
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