Magnetostratigraphy and cyclostratigraphy of the Tithonian interval from the Vaca Muerta Formation, southern Neuquén Basin, Argentina
A cyclostratigraphic and paleomagnetic study was carried out in the lower part of the Vaca Muerta Formation, Los Catutos Member (Lower to lowermost Upper Tithonian) at the southern region of the Sierra de la Vaca Muerta, Neuquén Basin, west-central Argentina. The Vaca Muerta Formation is known for i...
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2018
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| LEADER | 22551caa a22015017a 4500 | ||
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| 001 | PAPER-16840 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518204752.0 | ||
| 008 | 190410s2018 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-85047142466 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Kohan Martínez, M. | |
| 245 | 1 | 0 | |a Magnetostratigraphy and cyclostratigraphy of the Tithonian interval from the Vaca Muerta Formation, southern Neuquén Basin, Argentina |
| 260 | |b Elsevier Ltd |c 2018 | ||
| 270 | 1 | 0 | |m Kohan Martínez, M.; IGEBA - CONICET, Departamento de Cs. Geológicas, Facultad de ciencias exactas y naturales, Universidad de Buenos Aires, Pab. 2 Ciudad UniversitariaArgentina; email: melisa.kohan@gmail.com |
| 506 | |2 openaire |e Política editorial | ||
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| 520 | 3 | |a A cyclostratigraphic and paleomagnetic study was carried out in the lower part of the Vaca Muerta Formation, Los Catutos Member (Lower to lowermost Upper Tithonian) at the southern region of the Sierra de la Vaca Muerta, Neuquén Basin, west-central Argentina. The Vaca Muerta Formation is known for its unconventional resource potential and its exceptional behaviour as a world-class source rock. The studied section is c. 90 m thick and is characterized by decimetre-scale rhythmic alternations of marls, mudstones and limestones, showing a well-ordered hierarchy of cycles. Elementary cycles, bundles and superbundles were recognized with frequencies within the Milankovitch spectrum band. A total of 280 standard specimens collected from 35 paleomagnetic sampling horizons, dated with ammonites, were analyzed. The quality and primary origin of the characteristic magnetization was proved through the corresponding reversal test. A magnetostratigraphic scale was thus constructed that comprises 5 reverse and 4 normal polarity intervals, spanning the Andean Virgatosphinctes andesensis (ex mendozanus) (Lower Tithonian) to Windhauseniceras internispinosum (lowermost Upper Tithonian) ammonite Zones. Polarities were correlated with the GPTS 2016 using the equivalences between the Andean and Standard ammonite zones which, allowed to interpret that Los Catutos section was deposited between M22r to M20n Subchrons. By means of the correlation between the cyclostratigraphic and magnetostratigraphic scales, it was possible to date the Tithonian succession with unprecedented precision. Rock magnetic studies indicate that the remanence is carried by titanomagnetite. © 2018 Elsevier Ltd |l eng | |
| 536 | |a Detalles de la financiación: Universidad de Buenos Aires | ||
| 536 | |a Detalles de la financiación: Agencia Nacional de Promoción Científica y Tecnológica | ||
| 536 | |a Detalles de la financiación: Shell | ||
| 536 | |a Detalles de la financiación: National Council for Scientific Research | ||
| 536 | |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas | ||
| 536 | |a Detalles de la financiación: This research has been done under the framework of the PICT-2015-0206 and 2016–3762 projects supported by the Agencia Nacional de Promoción Científica y Tecnológica. We would like to specially thank to the Instituto de Astronomía, Geofísica e Ciências Atmosféricas (IAG) da Universidade de São Paulo (USP), Brasil, for their help and enormous generosity during the time we spent working there. Also, thanks to the National Scientific and Technical Research Council (CONICET) for the Phd scholarship and to the University of Buenos Aires (UBA) for the high quality education and the work-space provided. We are deeply thankful with the valuable reviews of James Ogg and an anonymous reviewer, which allowed to improve the original manuscript. The results of this work were partially obtained with the financial support as part of the Vaca Muerta Consortium (Shell, Chevron and Total) of the University of Buenos Aires . Appendix A | ||
| 593 | |a Consejo Nacional de Investigaciones Científicas y Técnicas, Argentina | ||
| 593 | |a IGEBA, Depto. de Cs. Geológicas, Fac. de Cs. Exactas y Naturales, Universidad de Buenos Aires, Pab. 2 Ciudad Universitaria, Buenos Aires, C1428EHA, Argentina | ||
| 593 | |a MACNBR, Museo Argentino de Ciencias Naturales “Bernardino Rivadavia”, Av. Ángel Gallardo 490, CABA, C1405DJR, Argentina | ||
| 690 | 1 | 0 | |a CYCLOSTRATIGRAPHY |
| 690 | 1 | 0 | |a JURASSIC |
| 690 | 1 | 0 | |a MAGNETOSTRATIGRAPHY |
| 690 | 1 | 0 | |a TITHONIAN |
| 690 | 1 | 0 | |a VACA MUERTA |
| 690 | 1 | 0 | |a AMMONITE |
| 690 | 1 | 0 | |a CYCLOSTRATIGRAPHY |
| 690 | 1 | 0 | |a DATING METHOD |
| 690 | 1 | 0 | |a MAGNETIZATION |
| 690 | 1 | 0 | |a MAGNETOSTRATIGRAPHY |
| 690 | 1 | 0 | |a PALEOMAGNETISM |
| 690 | 1 | 0 | |a REMANENT MAGNETIZATION |
| 690 | 1 | 0 | |a SOURCE ROCK |
| 690 | 1 | 0 | |a STRATIGRAPHIC CORRELATION |
| 690 | 1 | 0 | |a TITHONIAN |
| 651 | 4 | |a ARGENTINA | |
| 651 | 4 | |a NEUQUEN BASIN | |
| 700 | 1 | |a Kietzmann, D.A. | |
| 700 | 1 | |a Iglesia Llanos, M.P. | |
| 700 | 1 | |a Leanza, H.A. | |
| 700 | 1 | |a Luppo, T. | |
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