2002
DOI: 10.1016/s0012-821x(02)00900-7
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Multivectorial paleointensity determination from the Cordova Gabbro, southern Ontario

Abstract: We report geomagnetic field intensities for the A (V1000 Ma) and B (V850 Ma) natural remanent magnetizations of the Cordova Gabbro of southern Ontario. We interpret A and B to be secondary thermal overprints produced during regional uplift and cooling following the Grenvillian Orogeny. Multivectorial A+B paleointensity data were analyzed using pairs of Arai diagrams for the separated A and B vectors. From 18 reliable A results and 15 reliable B results, we find paleofield values of 18.1 þ 2.1 WT and 7.1 þ 1.5 … Show more

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Cited by 55 publications
(59 citation statements)
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“…Additionally, the data consist of one single measurement only. At the same time, the data is in obvious contrast with reliable results recently obtained for the Cordova Gabbro (850 Myr) by Yu et al (2002), showing a VDM of 1.8 ± 0.4 10 22 Am 2 . The comparison with the other PINT03 data suggests that the intensities determined from Jänisjärvi are considerably biased towards higher values.…”
Section: Paleointensities and Virtual Dipole Momentcontrasting
confidence: 99%
“…Additionally, the data consist of one single measurement only. At the same time, the data is in obvious contrast with reliable results recently obtained for the Cordova Gabbro (850 Myr) by Yu et al (2002), showing a VDM of 1.8 ± 0.4 10 22 Am 2 . The comparison with the other PINT03 data suggests that the intensities determined from Jänisjärvi are considerably biased towards higher values.…”
Section: Paleointensities and Virtual Dipole Momentcontrasting
confidence: 99%
“…The lake sediments and gabbros used in this study had intermediate AF behavior, with about 50% of pARM demagnetizing over the field blocking range (Figure 4). They nevertheless have previously yielded successful paleointensity results by the pseudo‐Thellier and Thellier methods, respectively [ Brachfeld and Banerjee , 2000; Yu and Dunlop , 2001, 2002]. This success is rather surprising in view of their ambivalent behavior in pARM reciprocity experiments.…”
Section: Discussionmentioning
confidence: 99%
“…Relative intensities are plotted in Figure 7. For SD and PSD samples 1 (0.065 μm), 4 (0.24 μm), 5 (0.34 μm), 6 (1.06 μm), 456 A, 578 A, T 19, and C 12 (Cordova Gabbro, Ontario [ Yu and Dunlop , 2002]), the intensities of pARM n * and pARM n are almost identical. However, for large PSD and MD samples 9 (16.9 μm), 10 (18.3 μm), Bu 5, Bu 8, and S 50, pARM n * is 6–14% more intense than pARM n .…”
Section: Effect Of Magnetic Prehistory On Parmmentioning
confidence: 99%
“…Twenty‐eight natural samples were also studied: two andesites (An 1, An 3), one pumice (Na 2), one red scoria (Km 3) [ Yu , 1998], 14 gabbros [ Yu and Dunlop , 2001, 2002], three granites [ Dunlop , 1984; Dunlop et al , 1984], and seven freeze‐dried lake sediments [ Brachfeld and Banerjee , 2000]. The natural samples selected have magnetic and paleomagnetic properties that are well documented.…”
Section: Samplesmentioning
confidence: 99%
“…They were chosen from a much larger collection of several hundred cores on the basis of their low magnetic fabric anisotropy, their reproducible ARM and TRM intensities (ARM only for sediments), and minimal viscous magnetic changes. The gabbros [ Yu and Dunlop , 2001, 2002] and lake sediments [ Brachfeld and Banerjee , 2000] had yielded reliable paleointensities by the Thellier and pseudo‐Thellier methods, respectively.…”
Section: Samplesmentioning
confidence: 99%