Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate
Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan V...
Ausführliche Beschreibung
Autor*in: |
Sangode, S J [verfasserIn] |
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Format: |
E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
2022 |
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Schlagwörter: |
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Anmerkung: |
© Indian Academy of Sciences 2022 |
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Übergeordnetes Werk: |
Enthalten in: Journal of earth system science - Bangalore : Indian Acad. of Sciences, 1980, 131(2022), 3 vom: 12. Aug. |
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Übergeordnetes Werk: |
volume:131 ; year:2022 ; number:3 ; day:12 ; month:08 |
Links: |
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DOI / URN: |
10.1007/s12040-022-01917-x |
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Katalog-ID: |
SPR047834749 |
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520 | |a Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan Volcanic Province discovered an inclination anomaly of +10 degrees during the Deccan main phase eruptions ($ DE_{M} $ within Chron C29r at 66.398–65.688 Ma). The anomaly represents northward tilt during C29r followed by its restoration in C29n (~65 Ma). This anomaly is explained here by the Indian lithospheric response to Réunion plume head during $ DE_{M} $. A sequence of coincident geodynamic instances including: (i) biostratigraphically constrained ‘the brief inland seaway’, (ii) development of a regional southward dip for the lava flows, (iii) major drop in sea level at the southern tip of peninsula, and (iv) accelerated spreading and convergence rates during C29r to 29n transitions; substantiate the effect of lithospheric tilt and its restoration. We present a plume-lithosphere evolutionary model to explain the anomaly and its wider implications over the Indian lithospheric plate. | ||
650 | 4 | |a Deccan traps |7 (dpeaa)DE-He213 | |
650 | 4 | |a palaeomagnetism |7 (dpeaa)DE-He213 | |
650 | 4 | |a Indian plate |7 (dpeaa)DE-He213 | |
650 | 4 | |a Réunion hotspot |7 (dpeaa)DE-He213 | |
650 | 4 | |a Late Cretaceous |7 (dpeaa)DE-He213 | |
700 | 1 | |a Dongre, Ashish |4 aut | |
700 | 1 | |a Bhagat, Amarjeet |4 aut | |
700 | 1 | |a Meshram, Dhananjay |4 aut | |
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10.1007/s12040-022-01917-x doi (DE-627)SPR047834749 (SPR)s12040-022-01917-x-e DE-627 ger DE-627 rakwb eng Sangode, S J verfasserin aut Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Indian Academy of Sciences 2022 Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan Volcanic Province discovered an inclination anomaly of +10 degrees during the Deccan main phase eruptions ($ DE_{M} $ within Chron C29r at 66.398–65.688 Ma). The anomaly represents northward tilt during C29r followed by its restoration in C29n (~65 Ma). This anomaly is explained here by the Indian lithospheric response to Réunion plume head during $ DE_{M} $. A sequence of coincident geodynamic instances including: (i) biostratigraphically constrained ‘the brief inland seaway’, (ii) development of a regional southward dip for the lava flows, (iii) major drop in sea level at the southern tip of peninsula, and (iv) accelerated spreading and convergence rates during C29r to 29n transitions; substantiate the effect of lithospheric tilt and its restoration. We present a plume-lithosphere evolutionary model to explain the anomaly and its wider implications over the Indian lithospheric plate. Deccan traps (dpeaa)DE-He213 palaeomagnetism (dpeaa)DE-He213 Indian plate (dpeaa)DE-He213 Réunion hotspot (dpeaa)DE-He213 Late Cretaceous (dpeaa)DE-He213 Dongre, Ashish aut Bhagat, Amarjeet aut Meshram, Dhananjay aut Enthalten in Journal of earth system science Bangalore : Indian Acad. of Sciences, 1980 131(2022), 3 vom: 12. Aug. (DE-627)349877327 (DE-600)2081712-5 0973-774X nnns volume:131 year:2022 number:3 day:12 month:08 https://dx.doi.org/10.1007/s12040-022-01917-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 AR 131 2022 3 12 08 |
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10.1007/s12040-022-01917-x doi (DE-627)SPR047834749 (SPR)s12040-022-01917-x-e DE-627 ger DE-627 rakwb eng Sangode, S J verfasserin aut Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Indian Academy of Sciences 2022 Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan Volcanic Province discovered an inclination anomaly of +10 degrees during the Deccan main phase eruptions ($ DE_{M} $ within Chron C29r at 66.398–65.688 Ma). The anomaly represents northward tilt during C29r followed by its restoration in C29n (~65 Ma). This anomaly is explained here by the Indian lithospheric response to Réunion plume head during $ DE_{M} $. A sequence of coincident geodynamic instances including: (i) biostratigraphically constrained ‘the brief inland seaway’, (ii) development of a regional southward dip for the lava flows, (iii) major drop in sea level at the southern tip of peninsula, and (iv) accelerated spreading and convergence rates during C29r to 29n transitions; substantiate the effect of lithospheric tilt and its restoration. We present a plume-lithosphere evolutionary model to explain the anomaly and its wider implications over the Indian lithospheric plate. Deccan traps (dpeaa)DE-He213 palaeomagnetism (dpeaa)DE-He213 Indian plate (dpeaa)DE-He213 Réunion hotspot (dpeaa)DE-He213 Late Cretaceous (dpeaa)DE-He213 Dongre, Ashish aut Bhagat, Amarjeet aut Meshram, Dhananjay aut Enthalten in Journal of earth system science Bangalore : Indian Acad. of Sciences, 1980 131(2022), 3 vom: 12. Aug. (DE-627)349877327 (DE-600)2081712-5 0973-774X nnns volume:131 year:2022 number:3 day:12 month:08 https://dx.doi.org/10.1007/s12040-022-01917-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 AR 131 2022 3 12 08 |
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10.1007/s12040-022-01917-x doi (DE-627)SPR047834749 (SPR)s12040-022-01917-x-e DE-627 ger DE-627 rakwb eng Sangode, S J verfasserin aut Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Indian Academy of Sciences 2022 Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan Volcanic Province discovered an inclination anomaly of +10 degrees during the Deccan main phase eruptions ($ DE_{M} $ within Chron C29r at 66.398–65.688 Ma). The anomaly represents northward tilt during C29r followed by its restoration in C29n (~65 Ma). This anomaly is explained here by the Indian lithospheric response to Réunion plume head during $ DE_{M} $. A sequence of coincident geodynamic instances including: (i) biostratigraphically constrained ‘the brief inland seaway’, (ii) development of a regional southward dip for the lava flows, (iii) major drop in sea level at the southern tip of peninsula, and (iv) accelerated spreading and convergence rates during C29r to 29n transitions; substantiate the effect of lithospheric tilt and its restoration. We present a plume-lithosphere evolutionary model to explain the anomaly and its wider implications over the Indian lithospheric plate. Deccan traps (dpeaa)DE-He213 palaeomagnetism (dpeaa)DE-He213 Indian plate (dpeaa)DE-He213 Réunion hotspot (dpeaa)DE-He213 Late Cretaceous (dpeaa)DE-He213 Dongre, Ashish aut Bhagat, Amarjeet aut Meshram, Dhananjay aut Enthalten in Journal of earth system science Bangalore : Indian Acad. of Sciences, 1980 131(2022), 3 vom: 12. Aug. (DE-627)349877327 (DE-600)2081712-5 0973-774X nnns volume:131 year:2022 number:3 day:12 month:08 https://dx.doi.org/10.1007/s12040-022-01917-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 AR 131 2022 3 12 08 |
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10.1007/s12040-022-01917-x doi (DE-627)SPR047834749 (SPR)s12040-022-01917-x-e DE-627 ger DE-627 rakwb eng Sangode, S J verfasserin aut Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Indian Academy of Sciences 2022 Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan Volcanic Province discovered an inclination anomaly of +10 degrees during the Deccan main phase eruptions ($ DE_{M} $ within Chron C29r at 66.398–65.688 Ma). The anomaly represents northward tilt during C29r followed by its restoration in C29n (~65 Ma). This anomaly is explained here by the Indian lithospheric response to Réunion plume head during $ DE_{M} $. A sequence of coincident geodynamic instances including: (i) biostratigraphically constrained ‘the brief inland seaway’, (ii) development of a regional southward dip for the lava flows, (iii) major drop in sea level at the southern tip of peninsula, and (iv) accelerated spreading and convergence rates during C29r to 29n transitions; substantiate the effect of lithospheric tilt and its restoration. We present a plume-lithosphere evolutionary model to explain the anomaly and its wider implications over the Indian lithospheric plate. Deccan traps (dpeaa)DE-He213 palaeomagnetism (dpeaa)DE-He213 Indian plate (dpeaa)DE-He213 Réunion hotspot (dpeaa)DE-He213 Late Cretaceous (dpeaa)DE-He213 Dongre, Ashish aut Bhagat, Amarjeet aut Meshram, Dhananjay aut Enthalten in Journal of earth system science Bangalore : Indian Acad. of Sciences, 1980 131(2022), 3 vom: 12. Aug. (DE-627)349877327 (DE-600)2081712-5 0973-774X nnns volume:131 year:2022 number:3 day:12 month:08 https://dx.doi.org/10.1007/s12040-022-01917-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 AR 131 2022 3 12 08 |
allfieldsSound |
10.1007/s12040-022-01917-x doi (DE-627)SPR047834749 (SPR)s12040-022-01917-x-e DE-627 ger DE-627 rakwb eng Sangode, S J verfasserin aut Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Indian Academy of Sciences 2022 Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan Volcanic Province discovered an inclination anomaly of +10 degrees during the Deccan main phase eruptions ($ DE_{M} $ within Chron C29r at 66.398–65.688 Ma). The anomaly represents northward tilt during C29r followed by its restoration in C29n (~65 Ma). This anomaly is explained here by the Indian lithospheric response to Réunion plume head during $ DE_{M} $. A sequence of coincident geodynamic instances including: (i) biostratigraphically constrained ‘the brief inland seaway’, (ii) development of a regional southward dip for the lava flows, (iii) major drop in sea level at the southern tip of peninsula, and (iv) accelerated spreading and convergence rates during C29r to 29n transitions; substantiate the effect of lithospheric tilt and its restoration. We present a plume-lithosphere evolutionary model to explain the anomaly and its wider implications over the Indian lithospheric plate. Deccan traps (dpeaa)DE-He213 palaeomagnetism (dpeaa)DE-He213 Indian plate (dpeaa)DE-He213 Réunion hotspot (dpeaa)DE-He213 Late Cretaceous (dpeaa)DE-He213 Dongre, Ashish aut Bhagat, Amarjeet aut Meshram, Dhananjay aut Enthalten in Journal of earth system science Bangalore : Indian Acad. of Sciences, 1980 131(2022), 3 vom: 12. Aug. (DE-627)349877327 (DE-600)2081712-5 0973-774X nnns volume:131 year:2022 number:3 day:12 month:08 https://dx.doi.org/10.1007/s12040-022-01917-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 AR 131 2022 3 12 08 |
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Enthalten in Journal of earth system science 131(2022), 3 vom: 12. Aug. volume:131 year:2022 number:3 day:12 month:08 |
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Sangode, S J @@aut@@ Dongre, Ashish @@aut@@ Bhagat, Amarjeet @@aut@@ Meshram, Dhananjay @@aut@@ |
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Sangode, S J |
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Sangode, S J misc Deccan traps misc palaeomagnetism misc Indian plate misc Réunion hotspot misc Late Cretaceous Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate |
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Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate Deccan traps (dpeaa)DE-He213 palaeomagnetism (dpeaa)DE-He213 Indian plate (dpeaa)DE-He213 Réunion hotspot (dpeaa)DE-He213 Late Cretaceous (dpeaa)DE-He213 |
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Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate |
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Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate |
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Sangode, S J Dongre, Ashish Bhagat, Amarjeet Meshram, Dhananjay |
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palaeomagnetic inclination anomaly in the deccan traps and its geodynamic implications over the indian plate |
title_auth |
Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate |
abstract |
Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan Volcanic Province discovered an inclination anomaly of +10 degrees during the Deccan main phase eruptions ($ DE_{M} $ within Chron C29r at 66.398–65.688 Ma). The anomaly represents northward tilt during C29r followed by its restoration in C29n (~65 Ma). This anomaly is explained here by the Indian lithospheric response to Réunion plume head during $ DE_{M} $. A sequence of coincident geodynamic instances including: (i) biostratigraphically constrained ‘the brief inland seaway’, (ii) development of a regional southward dip for the lava flows, (iii) major drop in sea level at the southern tip of peninsula, and (iv) accelerated spreading and convergence rates during C29r to 29n transitions; substantiate the effect of lithospheric tilt and its restoration. We present a plume-lithosphere evolutionary model to explain the anomaly and its wider implications over the Indian lithospheric plate. © Indian Academy of Sciences 2022 |
abstractGer |
Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan Volcanic Province discovered an inclination anomaly of +10 degrees during the Deccan main phase eruptions ($ DE_{M} $ within Chron C29r at 66.398–65.688 Ma). The anomaly represents northward tilt during C29r followed by its restoration in C29n (~65 Ma). This anomaly is explained here by the Indian lithospheric response to Réunion plume head during $ DE_{M} $. A sequence of coincident geodynamic instances including: (i) biostratigraphically constrained ‘the brief inland seaway’, (ii) development of a regional southward dip for the lava flows, (iii) major drop in sea level at the southern tip of peninsula, and (iv) accelerated spreading and convergence rates during C29r to 29n transitions; substantiate the effect of lithospheric tilt and its restoration. We present a plume-lithosphere evolutionary model to explain the anomaly and its wider implications over the Indian lithospheric plate. © Indian Academy of Sciences 2022 |
abstract_unstemmed |
Rapid northward drift of the Indian plate during Deccan volcanism assumes a gradual equatorward shallowing of the paleomagnetic inclinations amongst subsequently younger lava flows. Compilation of palaeomagnetic database and using 1062 statistically significant site mean directions from the Deccan Volcanic Province discovered an inclination anomaly of +10 degrees during the Deccan main phase eruptions ($ DE_{M} $ within Chron C29r at 66.398–65.688 Ma). The anomaly represents northward tilt during C29r followed by its restoration in C29n (~65 Ma). This anomaly is explained here by the Indian lithospheric response to Réunion plume head during $ DE_{M} $. A sequence of coincident geodynamic instances including: (i) biostratigraphically constrained ‘the brief inland seaway’, (ii) development of a regional southward dip for the lava flows, (iii) major drop in sea level at the southern tip of peninsula, and (iv) accelerated spreading and convergence rates during C29r to 29n transitions; substantiate the effect of lithospheric tilt and its restoration. We present a plume-lithosphere evolutionary model to explain the anomaly and its wider implications over the Indian lithospheric plate. © Indian Academy of Sciences 2022 |
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title_short |
Palaeomagnetic inclination anomaly in the Deccan traps and its geodynamic implications over the Indian plate |
url |
https://dx.doi.org/10.1007/s12040-022-01917-x |
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author2 |
Dongre, Ashish Bhagat, Amarjeet Meshram, Dhananjay |
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Dongre, Ashish Bhagat, Amarjeet Meshram, Dhananjay |
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doi_str |
10.1007/s12040-022-01917-x |
up_date |
2024-07-03T15:18:23.188Z |
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|
score |
7.402011 |