Home > Research > Publications & Outputs > A geomagnetic polarity timescale for the Permia...

Electronic data

Links

Text available via DOI:

View graph of relations

A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries

Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSNChapter (peer-reviewed)

E-pub ahead of print

Standard

A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries. / Hounslow, Mark William; Balabanov, Yuri P.

The Permian timescale. ed. / Spencer Lucas; Shugong. Z. Shen. London : Geological Society of London, 2016. ( Geological Society, London, Special Publications; Vol. 450).

Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSNChapter (peer-reviewed)

Harvard

Hounslow, MW & Balabanov, YP 2016, A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries. in S Lucas & SZ Shen (eds), The Permian timescale. Geological Society, London, Special Publications, vol. 450, Geological Society of London, London. https://doi.org/10.1144/SP450.8

APA

Hounslow, M. W., & Balabanov, Y. P. (2016). A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries. In S. Lucas, & S. Z. Shen (Eds.), The Permian timescale ( Geological Society, London, Special Publications; Vol. 450). Geological Society of London. https://doi.org/10.1144/SP450.8

Vancouver

Hounslow MW, Balabanov YP. A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries. In Lucas S, Shen SZ, editors, The Permian timescale. London: Geological Society of London. 2016. ( Geological Society, London, Special Publications). https://doi.org/10.1144/SP450.8

Author

Hounslow, Mark William ; Balabanov, Yuri P. / A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries. The Permian timescale. editor / Spencer Lucas ; Shugong. Z. Shen. London : Geological Society of London, 2016. ( Geological Society, London, Special Publications).

Bibtex

@inbook{8ec5aaa525404182bdbc117f4f709654,
title = "A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries",
abstract = "The reverse polarity Kiaman Superchron has strong evidence for at least three, or prob ably four, normal magnetochrons during the early Permian. Normal magnetochrons are during the early Asselian (base CI1r.1n at 297.94+0.33 Ma), late Artinskian (CI2n at 281.24+2.3 Ma), mid-Kungurian (CI3n at 275.86+2.0 Ma) and Roadian (CI3r.an at 269.54+1.6 Ma). The mixed-polarity Illawarra Superchron begins in the early Wordian at 266.66+0.76 Ma. The Wordian–Capitanian interval is biased to normal polarity, but the basal Wuchiapingian begins the beginning of a significant reverse polarity magnetochron LP0r, with an overlying mixed-polarity interval through the later Lopingian. No significant magnetostratigraphic data gaps exist in the Permian geomagnetic polarity record. The early Cisuralian magnetochrons are calibrated to a succession of fusulinid zones, the later Cisuralian and Guadalupian to a conodont and fusulinid biostratigraphy, and Lopingian magnetochrons to conodont zonations. Age calibration of the magnetochrons is obtained through a Bayesian approach using 35 radiometric dates, and 95% confidence intervals on the ages and chron durations are obtained. The dating control points are most numerous in the Gzhelian–Asselian, Wordian and Changhsingian intervals. This significant advance should provide a framework for better correlation and dating of the marine and non-marine Permian",
author = "Hounslow, {Mark William} and Balabanov, {Yuri P.}",
year = "2016",
month = dec
day = "8",
doi = "10.1144/SP450.8",
language = "English",
series = " Geological Society, London, Special Publications",
publisher = "Geological Society of London",
editor = "Lucas, {Spencer } and Shen, {Shugong. Z. }",
booktitle = "The Permian timescale",
address = "United Kingdom",

}

RIS

TY - CHAP

T1 - A geomagnetic polarity timescale for the Permian, calibrated to stage boundaries

AU - Hounslow, Mark William

AU - Balabanov, Yuri P.

PY - 2016/12/8

Y1 - 2016/12/8

N2 - The reverse polarity Kiaman Superchron has strong evidence for at least three, or prob ably four, normal magnetochrons during the early Permian. Normal magnetochrons are during the early Asselian (base CI1r.1n at 297.94+0.33 Ma), late Artinskian (CI2n at 281.24+2.3 Ma), mid-Kungurian (CI3n at 275.86+2.0 Ma) and Roadian (CI3r.an at 269.54+1.6 Ma). The mixed-polarity Illawarra Superchron begins in the early Wordian at 266.66+0.76 Ma. The Wordian–Capitanian interval is biased to normal polarity, but the basal Wuchiapingian begins the beginning of a significant reverse polarity magnetochron LP0r, with an overlying mixed-polarity interval through the later Lopingian. No significant magnetostratigraphic data gaps exist in the Permian geomagnetic polarity record. The early Cisuralian magnetochrons are calibrated to a succession of fusulinid zones, the later Cisuralian and Guadalupian to a conodont and fusulinid biostratigraphy, and Lopingian magnetochrons to conodont zonations. Age calibration of the magnetochrons is obtained through a Bayesian approach using 35 radiometric dates, and 95% confidence intervals on the ages and chron durations are obtained. The dating control points are most numerous in the Gzhelian–Asselian, Wordian and Changhsingian intervals. This significant advance should provide a framework for better correlation and dating of the marine and non-marine Permian

AB - The reverse polarity Kiaman Superchron has strong evidence for at least three, or prob ably four, normal magnetochrons during the early Permian. Normal magnetochrons are during the early Asselian (base CI1r.1n at 297.94+0.33 Ma), late Artinskian (CI2n at 281.24+2.3 Ma), mid-Kungurian (CI3n at 275.86+2.0 Ma) and Roadian (CI3r.an at 269.54+1.6 Ma). The mixed-polarity Illawarra Superchron begins in the early Wordian at 266.66+0.76 Ma. The Wordian–Capitanian interval is biased to normal polarity, but the basal Wuchiapingian begins the beginning of a significant reverse polarity magnetochron LP0r, with an overlying mixed-polarity interval through the later Lopingian. No significant magnetostratigraphic data gaps exist in the Permian geomagnetic polarity record. The early Cisuralian magnetochrons are calibrated to a succession of fusulinid zones, the later Cisuralian and Guadalupian to a conodont and fusulinid biostratigraphy, and Lopingian magnetochrons to conodont zonations. Age calibration of the magnetochrons is obtained through a Bayesian approach using 35 radiometric dates, and 95% confidence intervals on the ages and chron durations are obtained. The dating control points are most numerous in the Gzhelian–Asselian, Wordian and Changhsingian intervals. This significant advance should provide a framework for better correlation and dating of the marine and non-marine Permian

U2 - 10.1144/SP450.8

DO - 10.1144/SP450.8

M3 - Chapter (peer-reviewed)

T3 - Geological Society, London, Special Publications

BT - The Permian timescale

A2 - Lucas, Spencer

A2 - Shen, Shugong. Z.

PB - Geological Society of London

CY - London

ER -