2020
DOI: 10.1016/j.epsl.2020.116071
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Timing and causes of the mid-Cretaceous global plate reorganization event

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Cited by 25 publications
(23 citation statements)
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“…The CNS (C34n; informally called “the Cretaceous quiet zone,” e.g., Gee & Kent, 2007) is a long period of nearly uniform normal polarity, first observed by Helsley and Steiner (1968) in ocean‐floor magnetic anomaly profiles. The CNS begins between 123.0 and 121.2 Ma, with a duration of 38.0–40.5 Ma (see review by Olierook et al., 2020), and it provides an opportunity to investigate the geomagnetic field behavior before, during, and after a superchron. Indeed, the CNS is preceded by the so‐called “Mesozoic dipole low” (Prèvot et al., 1990) with an average intensity value of ∼32 ZAm 2 (e.g., Tauxe et al., 2013), possibly linked to a change of state of the geomagnetic field from a state of relatively rapid reversals, to a period of stability during the CNS.…”
Section: The Cretaceous Normal Superchron (Cns)mentioning
confidence: 99%
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“…The CNS (C34n; informally called “the Cretaceous quiet zone,” e.g., Gee & Kent, 2007) is a long period of nearly uniform normal polarity, first observed by Helsley and Steiner (1968) in ocean‐floor magnetic anomaly profiles. The CNS begins between 123.0 and 121.2 Ma, with a duration of 38.0–40.5 Ma (see review by Olierook et al., 2020), and it provides an opportunity to investigate the geomagnetic field behavior before, during, and after a superchron. Indeed, the CNS is preceded by the so‐called “Mesozoic dipole low” (Prèvot et al., 1990) with an average intensity value of ∼32 ZAm 2 (e.g., Tauxe et al., 2013), possibly linked to a change of state of the geomagnetic field from a state of relatively rapid reversals, to a period of stability during the CNS.…”
Section: The Cretaceous Normal Superchron (Cns)mentioning
confidence: 99%
“…These in turn have significant implications for the geodynamo and mantle modeling (Biggin et al., 2012). Moreover, understanding the long‐term variations of the geomagnetic field strength (Ingham et al., 2014; Juarez et al., 1998; Kulakov et al., 2019; McFadden & McElhinny, 1982; Tauxe et al., 2013; Wang et al., 2015) over thousands to millions of years is not only fundamental for modeling the geodynamo origin and behavior (e.g., Biggin et al., 2012) but also for other applications, such as estimating the solar standoff distance (Tarduno et al., 2014) or geodynamic plate reconstructions (e.g., Olierook et al., 2020). However, there is no consensus yet as to the average strength of the geomagnetic field, with estimates ranging from 80 ± 7 ZAm 2 (where ZAm 2 = 10 21 Am 2 ) for the last 5 Ma (McFadden & McElhinny, 1982), to 42 ± 23 ZAm 2 for the last 160 Ma (all intensity values errors are 1σ; Juarez et al., 1998; Tauxe et al., 2013).…”
Section: Introductionmentioning
confidence: 99%
“…Data compiled from Adams et al (2016Adams et al ( , 2013 with minimum zircon grains n = 3, younger zircons where n < 3 not shown. Olierook et al, 2020;Schellart et al, 2006;Veevers, 2000;Zundel et al, 2019). Uncertainty remains, however, regarding the timing and manner of East Gondwanan subduction shut-down (and collision of the Hikurangi Plateau) with estimates ranging between 100 and 86 Ma based variously on mapping of sea-floor fabrics, stratigraphy, plate reconstructions, and geochronology (Barrett et al, 2018;Billen & Stock, 2000;Crampton et al, 2019;Davy, 2014;Kamp, 1999Kamp, , 2000Mazengarb & Harris, 1994;Mortimer et al, 2019;Müller et al, 2016).…”
Section: Geologic Backgroundmentioning
confidence: 99%
“…The CNS (C34n; informally called "the Cretaceous quiet zone," e.g., Gee & Kent, 2007) is a long period of nearly uniform normal polarity, first observed by Helsley and Steiner (1968) in ocean-floor magnetic anomaly profiles. The CNS begins between 123.0 and 121.2 Ma, with a duration of 38.0-40.5 Ma (see review by Olierook et al, 2020), and it provides an opportunity to investigate the geomagnetic field behavior before, during, and after a superchron. Indeed, the CNS is preceded by the so-called "Mesozoic dipole low" (Prèvot et al, 1990) with an average intensity value of ∼32 ZAm 2 (e.g., Tauxe et al, 2013), possibly linked to a change of state of the geomagnetic field from a state of relatively rapid reversals, to a period of stability during the CNS.…”
Section: The Cretaceous Normal Superchron (Cns)mentioning
confidence: 99%
“…These in turn have significant implications for the geodynamo and mantle modeling (Biggin et al, 2012). Moreover, understanding the long-term variations of the geomagnetic field strength (Ingham et al, 2014;Juarez et al, 1998;Kulakov et al, 2019;McFadden & McElhinny, 1982;Tauxe et al, 2013;Wang et al, 2015) over thousands to millions of years is not only fundamental for modeling the geodynamo origin and behavior (e.g., Biggin et al, 2012) but also for other applications, such as estimating the solar standoff distance (Tarduno et al, 2014) or geodynamic plate reconstructions (e.g., Olierook et al, 2020). However, there is no consensus yet as to the average strength of the geomagnetic field, with estimates ranging from 80 ± 7 ZAm 2 (where ZAm 2 = 10 21 Am 2 ) for the last 5 Ma (McFadden & McElhinny, 1982), to 42 ± 23 ZAm 2 for the last 160 Ma (all intensity values errors are 1σ; Juarez et al, 1998;Tauxe et al, 2013).…”
mentioning
confidence: 99%