Astronomical duration of polarity Chron C31r (lower Maastrichtian): cyclostratigraphy of the ODP Hole 762C (Indian Ocean) and the Contessa section (Italy)

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Standard

Astronomical duration of polarity Chron C31r (lower Maastrichtian) : cyclostratigraphy of the ODP Hole 762C (Indian Ocean) and the Contessa section (Italy). / Husson, Dorothee; Galbrun, Bruno; Thibault, Nicolas Rudolph; Gardin, Silvia; Huret, Emilia; Coccioni, Rodolfo.

I: Geological Magazine, Bind 149, Nr. 2, 2012, s. 345-351.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Husson, D, Galbrun, B, Thibault, NR, Gardin, S, Huret, E & Coccioni, R 2012, 'Astronomical duration of polarity Chron C31r (lower Maastrichtian): cyclostratigraphy of the ODP Hole 762C (Indian Ocean) and the Contessa section (Italy)', Geological Magazine, bind 149, nr. 2, s. 345-351. https://doi.org/10.1017/S0016756811000999

APA

Husson, D., Galbrun, B., Thibault, N. R., Gardin, S., Huret, E., & Coccioni, R. (2012). Astronomical duration of polarity Chron C31r (lower Maastrichtian): cyclostratigraphy of the ODP Hole 762C (Indian Ocean) and the Contessa section (Italy). Geological Magazine, 149(2), 345-351. https://doi.org/10.1017/S0016756811000999

Vancouver

Husson D, Galbrun B, Thibault NR, Gardin S, Huret E, Coccioni R. Astronomical duration of polarity Chron C31r (lower Maastrichtian): cyclostratigraphy of the ODP Hole 762C (Indian Ocean) and the Contessa section (Italy). Geological Magazine. 2012;149(2):345-351. https://doi.org/10.1017/S0016756811000999

Author

Husson, Dorothee ; Galbrun, Bruno ; Thibault, Nicolas Rudolph ; Gardin, Silvia ; Huret, Emilia ; Coccioni, Rodolfo. / Astronomical duration of polarity Chron C31r (lower Maastrichtian) : cyclostratigraphy of the ODP Hole 762C (Indian Ocean) and the Contessa section (Italy). I: Geological Magazine. 2012 ; Bind 149, Nr. 2. s. 345-351.

Bibtex

@article{9fdf4e68ab894771bfedd0736454a9c7,
title = "Astronomical duration of polarity Chron C31r (lower Maastrichtian): cyclostratigraphy of the ODP Hole 762C (Indian Ocean) and the Contessa section (Italy)",
abstract = "The duration of polarity Chron C31r is estimated with a cyclostratigraphic approach. Two sites are investigated: ODP Site 762 (Indian Ocean) and the Contessa Highway section (Gubbio, Italy). Cyclostratigraphic analysis is performed on greyscale variations (Site 762) and magnetic susceptibility variations (Contessa section). Both sites reveal an astronomical control of the sedimentation, highlighted by the identification of all the orbital periodicities. Cyclostratigraphic signals are tuned on 405 ka eccentricity cycles extracted from the La04 astronomical solution. In both sites, cycle counting gives an estimate of the duration of polarity Chron C31r of about 2.09 ± 0.03 Ma. ",
author = "Dorothee Husson and Bruno Galbrun and Thibault, {Nicolas Rudolph} and Silvia Gardin and Emilia Huret and Rodolfo Coccioni",
year = "2012",
doi = "10.1017/S0016756811000999",
language = "English",
volume = "149",
pages = "345--351",
journal = "Geological Magazine",
issn = "0016-7568",
publisher = "Cambridge University Press",
number = "2",

}

RIS

TY - JOUR

T1 - Astronomical duration of polarity Chron C31r (lower Maastrichtian)

T2 - cyclostratigraphy of the ODP Hole 762C (Indian Ocean) and the Contessa section (Italy)

AU - Husson, Dorothee

AU - Galbrun, Bruno

AU - Thibault, Nicolas Rudolph

AU - Gardin, Silvia

AU - Huret, Emilia

AU - Coccioni, Rodolfo

PY - 2012

Y1 - 2012

N2 - The duration of polarity Chron C31r is estimated with a cyclostratigraphic approach. Two sites are investigated: ODP Site 762 (Indian Ocean) and the Contessa Highway section (Gubbio, Italy). Cyclostratigraphic analysis is performed on greyscale variations (Site 762) and magnetic susceptibility variations (Contessa section). Both sites reveal an astronomical control of the sedimentation, highlighted by the identification of all the orbital periodicities. Cyclostratigraphic signals are tuned on 405 ka eccentricity cycles extracted from the La04 astronomical solution. In both sites, cycle counting gives an estimate of the duration of polarity Chron C31r of about 2.09 ± 0.03 Ma.

AB - The duration of polarity Chron C31r is estimated with a cyclostratigraphic approach. Two sites are investigated: ODP Site 762 (Indian Ocean) and the Contessa Highway section (Gubbio, Italy). Cyclostratigraphic analysis is performed on greyscale variations (Site 762) and magnetic susceptibility variations (Contessa section). Both sites reveal an astronomical control of the sedimentation, highlighted by the identification of all the orbital periodicities. Cyclostratigraphic signals are tuned on 405 ka eccentricity cycles extracted from the La04 astronomical solution. In both sites, cycle counting gives an estimate of the duration of polarity Chron C31r of about 2.09 ± 0.03 Ma.

U2 - 10.1017/S0016756811000999

DO - 10.1017/S0016756811000999

M3 - Journal article

VL - 149

SP - 345

EP - 351

JO - Geological Magazine

JF - Geological Magazine

SN - 0016-7568

IS - 2

ER -

ID: 44357875