1984
DOI: 10.1016/0012-821x(84)90162-6
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Jurassic magnetic stratigraphy from Umbrian (Italian) land sections

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Cited by 39 publications
(7 citation statements)
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“…Magnetostratigraphic studies from condensed pelagic limestones at Bakonycsernye (Márton et al, 1980), Fonte Avellana and Cingoli (Channell et al,1984) show a dominance of reverse polarity across the Sinemurian-Pliensbachian boundary, in stark contrast to results presented here. This may be because the chronostratigraphy in these sections has both poor biostratigraphic control and hiatuses in the thin pelagic limestone successions may be frequent, as suggested by Opdyke and Channel (1996).…”
Section: And the Late Sinemurian Succession In The Montcornetcontrasting
confidence: 99%
“…Magnetostratigraphic studies from condensed pelagic limestones at Bakonycsernye (Márton et al, 1980), Fonte Avellana and Cingoli (Channell et al,1984) show a dominance of reverse polarity across the Sinemurian-Pliensbachian boundary, in stark contrast to results presented here. This may be because the chronostratigraphy in these sections has both poor biostratigraphic control and hiatuses in the thin pelagic limestone successions may be frequent, as suggested by Opdyke and Channel (1996).…”
Section: And the Late Sinemurian Succession In The Montcornetcontrasting
confidence: 99%
“…Sedimentation began in the Triassic as volcanic and coarse-grained continental deposits, and from the Late Triassic onwards a narrow marine corridor settled in the northern area of the basin. This sea expanded Fonte Avellana: [38]. GAOHVTH 94: [1]; O 95: [2,3].…”
Section: Geological Setting and Sampling Methodologymentioning
confidence: 99%
“…Sea-surface magnetic anomalies within the JQZ, arbitrarily delineated as older than anomaly M25, typically have very low amplitudes and there is a gradual increase in amplitude, extending from at least M29 to around M19, which may be field related (Cande et al, 1978;McElhinny and Larson, 2003) (Figure 8(a)). Although the lineated nature of even older M-sequence anomalies has been documented over fast spreading crust and used for tectonic reconstructions (Handschumacher et al, 1988;Nakanishi et al, 1989;Nakanishi and Winterer, 1998), magnetostratigraphic evidence for polarity reversals over the time interval represented by the JQZ, that is, prior to $M25, is still ambiguous (e.g., Channell et al, 1984;Juarez et al, 1994;Steiner et al, 1985). These older anomalies resemble the kind of shortwavelength, low-amplitude anomalies observed in the Cenozoic that have been attributed to paleointensity variations (Cande and Kent, 1992b).…”
Section: Source Of Oceanic Magnetic Anomalies and The Geomagnetic Polmentioning
confidence: 99%