Mechanisms of mud extrusion on the Mediterranean Ridge Accretionary Complex
Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence...
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| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1998 |
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| Umfang: |
18 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: Geo-marine letters - 1984, 18(1998) vom: Feb., Seite 97-114 |
| Übergeordnetes Werk: |
volume:18 ; year:1998 ; month:02 ; pages:97-114 ; extent:18 |
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| 520 | |a Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence can be deduced for both domes. Results from permeability and shear strength tests, grain size analyses, sedimentary textures, and clast provenance provide clues concerning the mechanism of mud volcanism. The collision of Africa with Eurasia resulted in backthrusting of the evaporite-dominated accretionary wedge against a rigid backstop. This allowed egress of overpressured fluid-rich mud of presumed Messinian age from the décollement, although many of the clasts may have originated from the overlying accretionary wedge. | ||
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| 700 | 1 | |a Flecker, R. |4 oth | |
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(DE-627)NLEJ203445686 DE-627 ger DE-627 rakwb eng Mechanisms of mud extrusion on the Mediterranean Ridge Accretionary Complex 1998 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence can be deduced for both domes. Results from permeability and shear strength tests, grain size analyses, sedimentary textures, and clast provenance provide clues concerning the mechanism of mud volcanism. The collision of Africa with Eurasia resulted in backthrusting of the evaporite-dominated accretionary wedge against a rigid backstop. This allowed egress of overpressured fluid-rich mud of presumed Messinian age from the décollement, although many of the clasts may have originated from the overlying accretionary wedge. Springer Online Journal Archives 1860-2002 Kopf, A. oth Robertson, A. H. F. oth Clennell, M. B. oth Flecker, R. oth in Geo-marine letters 1984 18(1998) vom: Feb., Seite 97-114 (DE-627)NLEJ188990755 (DE-600)1481423-7 1432-1157 nnns volume:18 year:1998 month:02 pages:97-114 extent:18 http://dx.doi.org/10.1007/s003670050058 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 18 1998 2 97-114 18 |
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(DE-627)NLEJ203445686 DE-627 ger DE-627 rakwb eng Mechanisms of mud extrusion on the Mediterranean Ridge Accretionary Complex 1998 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence can be deduced for both domes. Results from permeability and shear strength tests, grain size analyses, sedimentary textures, and clast provenance provide clues concerning the mechanism of mud volcanism. The collision of Africa with Eurasia resulted in backthrusting of the evaporite-dominated accretionary wedge against a rigid backstop. This allowed egress of overpressured fluid-rich mud of presumed Messinian age from the décollement, although many of the clasts may have originated from the overlying accretionary wedge. Springer Online Journal Archives 1860-2002 Kopf, A. oth Robertson, A. H. F. oth Clennell, M. B. oth Flecker, R. oth in Geo-marine letters 1984 18(1998) vom: Feb., Seite 97-114 (DE-627)NLEJ188990755 (DE-600)1481423-7 1432-1157 nnns volume:18 year:1998 month:02 pages:97-114 extent:18 http://dx.doi.org/10.1007/s003670050058 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 18 1998 2 97-114 18 |
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(DE-627)NLEJ203445686 DE-627 ger DE-627 rakwb eng Mechanisms of mud extrusion on the Mediterranean Ridge Accretionary Complex 1998 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence can be deduced for both domes. Results from permeability and shear strength tests, grain size analyses, sedimentary textures, and clast provenance provide clues concerning the mechanism of mud volcanism. The collision of Africa with Eurasia resulted in backthrusting of the evaporite-dominated accretionary wedge against a rigid backstop. This allowed egress of overpressured fluid-rich mud of presumed Messinian age from the décollement, although many of the clasts may have originated from the overlying accretionary wedge. Springer Online Journal Archives 1860-2002 Kopf, A. oth Robertson, A. H. F. oth Clennell, M. B. oth Flecker, R. oth in Geo-marine letters 1984 18(1998) vom: Feb., Seite 97-114 (DE-627)NLEJ188990755 (DE-600)1481423-7 1432-1157 nnns volume:18 year:1998 month:02 pages:97-114 extent:18 http://dx.doi.org/10.1007/s003670050058 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 18 1998 2 97-114 18 |
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(DE-627)NLEJ203445686 DE-627 ger DE-627 rakwb eng Mechanisms of mud extrusion on the Mediterranean Ridge Accretionary Complex 1998 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence can be deduced for both domes. Results from permeability and shear strength tests, grain size analyses, sedimentary textures, and clast provenance provide clues concerning the mechanism of mud volcanism. The collision of Africa with Eurasia resulted in backthrusting of the evaporite-dominated accretionary wedge against a rigid backstop. This allowed egress of overpressured fluid-rich mud of presumed Messinian age from the décollement, although many of the clasts may have originated from the overlying accretionary wedge. Springer Online Journal Archives 1860-2002 Kopf, A. oth Robertson, A. H. F. oth Clennell, M. B. oth Flecker, R. oth in Geo-marine letters 1984 18(1998) vom: Feb., Seite 97-114 (DE-627)NLEJ188990755 (DE-600)1481423-7 1432-1157 nnns volume:18 year:1998 month:02 pages:97-114 extent:18 http://dx.doi.org/10.1007/s003670050058 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 18 1998 2 97-114 18 |
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(DE-627)NLEJ203445686 DE-627 ger DE-627 rakwb eng Mechanisms of mud extrusion on the Mediterranean Ridge Accretionary Complex 1998 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence can be deduced for both domes. Results from permeability and shear strength tests, grain size analyses, sedimentary textures, and clast provenance provide clues concerning the mechanism of mud volcanism. The collision of Africa with Eurasia resulted in backthrusting of the evaporite-dominated accretionary wedge against a rigid backstop. This allowed egress of overpressured fluid-rich mud of presumed Messinian age from the décollement, although many of the clasts may have originated from the overlying accretionary wedge. Springer Online Journal Archives 1860-2002 Kopf, A. oth Robertson, A. H. F. oth Clennell, M. B. oth Flecker, R. oth in Geo-marine letters 1984 18(1998) vom: Feb., Seite 97-114 (DE-627)NLEJ188990755 (DE-600)1481423-7 1432-1157 nnns volume:18 year:1998 month:02 pages:97-114 extent:18 http://dx.doi.org/10.1007/s003670050058 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 18 1998 2 97-114 18 |
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Mechanisms of mud extrusion on the Mediterranean Ridge Accretionary Complex |
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Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence can be deduced for both domes. Results from permeability and shear strength tests, grain size analyses, sedimentary textures, and clast provenance provide clues concerning the mechanism of mud volcanism. The collision of Africa with Eurasia resulted in backthrusting of the evaporite-dominated accretionary wedge against a rigid backstop. This allowed egress of overpressured fluid-rich mud of presumed Messinian age from the décollement, although many of the clasts may have originated from the overlying accretionary wedge. |
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Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence can be deduced for both domes. Results from permeability and shear strength tests, grain size analyses, sedimentary textures, and clast provenance provide clues concerning the mechanism of mud volcanism. The collision of Africa with Eurasia resulted in backthrusting of the evaporite-dominated accretionary wedge against a rigid backstop. This allowed egress of overpressured fluid-rich mud of presumed Messinian age from the décollement, although many of the clasts may have originated from the overlying accretionary wedge. |
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Abstract Drilling two mud domes on the Mediterranean Ridge during ODP Leg 160 has demonstrated that the eruption of mud breccia began at least 1.5 Ma ago. An evolution through extrusive building of a cone, followed by successive eruptions of clast-bearing mud debris flows and subsequent subsidence can be deduced for both domes. Results from permeability and shear strength tests, grain size analyses, sedimentary textures, and clast provenance provide clues concerning the mechanism of mud volcanism. The collision of Africa with Eurasia resulted in backthrusting of the evaporite-dominated accretionary wedge against a rigid backstop. This allowed egress of overpressured fluid-rich mud of presumed Messinian age from the décollement, although many of the clasts may have originated from the overlying accretionary wedge. |
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