A paleomagnetic study of secular variation in New Zealand

1969 ◽  
Vol 6 (4) ◽  
pp. 257-267 ◽  
Author(s):  
Allan Cox
Keyword(s):  
New Zealand ◽  
Secular Variation ◽  
Paleomagnetic Study

New paleomagnetic results of the earliest Permian dykes in South Mongolia and their implications for the paleogeography of the Eastern CAOB

2021 ◽  
Author(s):  
Donghai Zhang ◽  
Guochun Zhao ◽  
Baochun Huang ◽  
Qian Zhao ◽  
Hai Zhou ◽  
...  
Keyword(s):  
Secular Variation ◽  
North China ◽  
High Coercivity ◽  
The North ◽  
Magnetic Carriers ◽  
Central Asian ◽  
Paleomagnetic Study ◽  
History Of ◽  
Temperature Component ◽  
Funded Project

<p>Debates of the Permo-Carboniferous paleogeography of the eastern Central Asian Orogenic Belt (CAOB) mainly focus on the existence, extent, and thereby evolutionary history of the Paleo-Asian Ocean (PAO) in this period. South Mongolia locates at a key position that denotes the southernmost margin of the Mongolia block. Here, we present a paleomagnetic study on the earliest Permian dykes near the Khanbogd of South Gobi Province in Mongolia to better constrain the paleo-position of the Mongolia block. Zircon U-Pb dating results of the studied dykes indicate an emplacement age of 299 ± 3 Ma. Magnetites are the dominant magnetic carriers as revealed by the synthesized rock magnetic experiments. A likely primary high coercivity/temperature component was isolated from 66 of 125 samples and displays consistent reverse polarity, which coincides with the Kiaman Reverse Superchron that overlapping the emplacement age of our studied dykes. Accordingly, a ~299 Ma paleomagnetic pole is calculated at <em>λ</em>/<em>φ</em> = −4.1°N/146.3°E (<em>dp</em> = 3.8, <em>dm</em> = 5.8, n = 66). Potential influence from Paleo-Secular Variation (PSV) is excluded following the Deenen et al. (2011) procedure. Our new results present a ~30.9°N paleolatitude for the Mongolia block, which differs from the lower paleolatitude of the North China and Xilinhot blocks as well as the much higher paleolititude of Siberia. Surrounded by these blocks of different paleolatitude, the PAO and Mongol-Okhotsk Ocean both remained wide open at least by the earliest Permian.</p><p><strong>Acknowledgments<br></strong>This research was funded by the Natural Science Foundation of China (NSFC) (41902229, 41730213, 42072264, 41902229, 41972237), China Postdoctoral Science Foundation funded project and Hong Kong RGC GRF (17307918).</p><p><strong>References</strong></p><p>Deenen, M. H. L. , Langereis, C. G. , Van, H. D. J. J. , & Biggin, A. J. . (2011). Geomagnetic secular variation and the statistics of palaeomagnetic directions. Geophysical Journal International(2), 509-520.</p><p></p><p></p>

A new high-resolution record of Holocene geomagnetic secular variation from New Zealand

2015 ◽  
Vol 430 ◽  
pp. 296-307 ◽  
Author(s):  
G.M. Turner ◽  
J.D. Howarth ◽  
G.I.N.O. de Gelder ◽  
S.J. Fitzsimons
Keyword(s):  
New Zealand ◽  
High Resolution ◽  
Secular Variation ◽  
Geomagnetic Secular Variation

500,000-Year Paleomagnetic Record from New Zealand Loess

1990 ◽  
Vol 33 (2) ◽  
pp. 178-187 ◽  
Author(s):  
Brad Pillans ◽  
Ian Wright
Keyword(s):  
New Zealand ◽  
Southern Hemisphere ◽  
Secular Variation ◽  
The Core ◽  
Rhyolitic Tephra

AbstractA paleomagnetic record of secular variation has been obtained from a 17.4-m-long core drilled from loess in North Island, New Zealand. Three dated rhyolitic tephra occur in the loess core at depths of 1.5, 3.4,and 13.0 m, with ages of 22,500, ≧42,000, and 370,000 years, respectively. The base of the core is estimated to be 500,000 years old, which makes this the longest continuous loess sequence yet described from the Southern Hemisphere. Two periods of anomalously low inclination in the core are correlated with the Mungo Event (ca. 35,000 years ago) and the Emperor Event (ca. 490,000 years ago); the Blake Event (ca. 115,000 years ago) is not recorded.

Magellanic Cloud Eclipsing Binaries: Primary Distance Indicators

1999 ◽  
Vol 190 ◽  
pp. 563-566
Author(s):  
J. D. Pritchard ◽  
W. Tobin ◽  
J. V. Clausen ◽  
E. F. Guinan ◽  
E. L. Fitzpatrick ◽  
...  
Keyword(s):  
New Zealand ◽  
Magellanic Cloud ◽  
Eclipsing Binaries ◽  
Fundamental Parameters ◽  
Distance Indicators

Our collaboration involves groups in Denmark, the U.S.A. Spain and of course New Zealand. Combining ground-based and satellite (IUEandHST) observations we aim to determine accurate and precise stellar fundamental parameters for the components of Magellanic Cloud Eclipsing Binaries as well as the distances to these systems and hence the parent galaxies themselves. This poster presents our latest progress.

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