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(a) The aligned RPI slope record from RS15-LC42 and the PISO-1500 10 kyr moving average, both standardised to a mean of 0 and SD of 1. The Geomagnetic Polarity Time Series is appended below, with normal polarity chrons displayed in black, and reverse polarity chrons displayed in white. (b) Downcore plot of the RPI slope from RS15-LC42. Black points indicate the data which was used for the Match protocol, with red crosses showing data that was excluded according to acceptable thresholds in R-Value, maximum angular deviation (MAD), and demagnetization behavior. (c) RPI slope R-value, displaying the correlation coefficient between NRM and ARM at AF strengths between 0 and 40 mT. A threshold of 0.9 was defined, with the corresponding RPI slope data of all points below this threshold being excluded from the RPI-PISO match procedure. (d) The MAD of principal component analysis (PCA). Red crosses indicate data above an acceptable data threshold of 15 • (red dashed line), with all data above this value excluded from the RPI-PISO match procedure. (e) The Characteristic Remnant Magnetisation (ChRM) inclination of PCA, which aligns with the expected inclination of 80.7 • reversed polarity, and 80.7 • normal polarity. (f) The newly revised age model (solid black line) compared to the existing age model of Ohneiser et al., 2019 (dashed black line). The black triangle displays the FO of Thalassiosira antarctica between 5.40 and 5.64 mbsf at 0.65 Ma. The undulating line at 9.34 mbsf marks the interpreted hiatus spanning the C1r.1n Jamarillo subchron, with the light grey dashed lines linking the fundamental initial age control of 0.781 Ma at 8.26 mbsf, defined by the Bruhnes-Maruyama magnetic reversal. (For interpretation of the references to colour in this figure legend, the reader is referred to the web version of this article.)

(a) The aligned RPI slope record from RS15-LC42 and the PISO-1500 10 kyr moving average, both standardised to a mean of 0 and SD of 1. The Geomagnetic Polarity Time Series is appended below, with normal polarity chrons displayed in black, and reverse polarity chrons displayed in white. (b) Downcore plot of the RPI slope from RS15-LC42. Black points indicate the data which was used for the Match protocol, with red crosses showing data that was excluded according to acceptable thresholds in R-Value, maximum angular deviation (MAD), and demagnetization behavior. (c) RPI slope R-value, displaying the correlation coefficient between NRM and ARM at AF strengths between 0 and 40 mT. A threshold of 0.9 was defined, with the corresponding RPI slope data of all points below this threshold being excluded from the RPI-PISO match procedure. (d) The MAD of principal component analysis (PCA). Red crosses indicate data above an acceptable data threshold of 15 • (red dashed line), with all data above this value excluded from the RPI-PISO match procedure. (e) The Characteristic Remnant Magnetisation (ChRM) inclination of PCA, which aligns with the expected inclination of 80.7 • reversed polarity, and 80.7 • normal polarity. (f) The newly revised age model (solid black line) compared to the existing age model of Ohneiser et al., 2019 (dashed black line). The black triangle displays the FO of Thalassiosira antarctica between 5.40 and 5.64 mbsf at 0.65 Ma. The undulating line at 9.34 mbsf marks the interpreted hiatus spanning the C1r.1n Jamarillo subchron, with the light grey dashed lines linking the fundamental initial age control of 0.781 Ma at 8.26 mbsf, defined by the Bruhnes-Maruyama magnetic reversal. (For interpretation of the references to colour in this figure legend, the reader is referred to the web version of this article.)

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Understanding how ocean circulation has varied around Antarctica in the past is vital because significant volumes of ice are grounded below sea level, and therefore ice sheet variations are strongly coupled with oceanographic variability at the continental shelf margin. This study investigates the 11.75 m sediment core RS15-LC42, retrieved from the...

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... was normalised by ARM to generate the RPI estimate. Fig. 4a displays a low WTC between the normaliser (ARM) and the RPI estimate of RS15-LC42. The newly revised age model is presented in Fig. 5, with the standardised output of the Match protocol displayed in Fig. 5a. A strong WTC between the aligned RPI estimate and PISO-1500 is observed in >20 kyr periods (Fig. 4b). Between the core-top and the B-M magnetic reversal at 8.26 m, all major peaks and troughs correspond between the RPI estimate of RS15-LC42 and the PISO-1500 ...
Context 2
... was normalised by ARM to generate the RPI estimate. Fig. 4a displays a low WTC between the normaliser (ARM) and the RPI estimate of RS15-LC42. The newly revised age model is presented in Fig. 5, with the standardised output of the Match protocol displayed in Fig. 5a. A strong WTC between the aligned RPI estimate and PISO-1500 is observed in >20 kyr periods (Fig. 4b). Between the core-top and the B-M magnetic reversal at 8.26 m, all major peaks and troughs correspond between the RPI estimate of RS15-LC42 and the PISO-1500 global stack. Below the B-M magnetic reversal (0.781 Ma) at 8.26 m, all ...

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Article
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