2021
DOI: 10.1029/2020jb021136
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A New Middle to Late Jurassic Geomagnetic Polarity Time Scale (GPTS) From a Multiscale Marine Magnetic Anomaly Survey of the Pacific Jurassic Quiet Zone

Abstract: Seafloor spreading marine magnetic anomalies provide the most continuous and comprehensive record of past geomagnetic field behavior extending back in time to ∼180 Ma. This record enables us to better understand the approximate locations and timing of the formation of new tectonic plates from the breakup of the supercontinent Pangea (e.g.

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Cited by 7 publications
(2 citation statements)
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“…Between ~150 Ma and ~110 Ma, Larson and Chase (1972) revealed that there are reversal periods sandwiched between periods of normal polarity (KQZ and the Jurassic Quiet Zone, JQZ). In fact, during the JQZ, geomagnetic reversals were frequent and the geomagnetic intensity was weak, as shown by MMA (e.g., Tominaga et al, 2021) and the absolute paleomagnetic intensity (paleointensity) of volcanic rocks (e.g., Tauxe et al, 2013). Larson and Pitman (1972) pointed out that the CNS corresponded in time to the KQZ of previous studies (e.g., Helsley and Steiner, 1968), designating C34n as the KQZ.…”
Section: Its Discoverymentioning
confidence: 80%
“…Between ~150 Ma and ~110 Ma, Larson and Chase (1972) revealed that there are reversal periods sandwiched between periods of normal polarity (KQZ and the Jurassic Quiet Zone, JQZ). In fact, during the JQZ, geomagnetic reversals were frequent and the geomagnetic intensity was weak, as shown by MMA (e.g., Tominaga et al, 2021) and the absolute paleomagnetic intensity (paleointensity) of volcanic rocks (e.g., Tauxe et al, 2013). Larson and Pitman (1972) pointed out that the CNS corresponded in time to the KQZ of previous studies (e.g., Helsley and Steiner, 1968), designating C34n as the KQZ.…”
Section: Its Discoverymentioning
confidence: 80%
“…Over timescales of ∼10 5 –10 8 years, the geomagnetic field's intensity appears to display an inverse relationship with its polarity reversal frequency (Driscoll & Olson, 2009; Glatzmaier et al., 1999; Hawkins et al., 2021; Tarduno & Cottrell, 2005; Tauxe, 2006; Tauxe & Hartl, 1997; Valet et al., 2005), which may represent a fundamental property of the geodynamo (Smirnov et al., 2017). Although low field intensities during frequent reversals have been widely recognized (e.g., Biggin et al., 2012; McElhinny & Larson, 2003; Tauxe et al., 2013; Tominaga et al., 2021), the geomagnetic field behaviors during long intervals of nearly no polarity reversals, that is, superchrons, remain poorly characterized and understood (e.g., Brandt et al., 2021; Cottrell et al., 2008; Zhang et al., 2021). In particular, it is not well known as to whether geomagnetic field strength stayed persistently strong/weak or exhibited some form of variations during a superchron.…”
Section: Introductionmentioning
confidence: 99%