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CORRECTION article

Front. Earth Sci., 11 July 2022
Sec. Structural Geology and Tectonics

Corrigendum: New Paleomagnetic Constraints on the Early Cretaceous Paleolatitude of the Lhasa Terrane (Tibet)

Zhenyu Li,
Zhenyu Li1,2*Lin Ding,,Lin Ding1,2,3Andrew K. Laskowski,Andrew K. Laskowski4,5William B. BurkeWilliam B. Burke4Yaofei ChenYaofei Chen6Peiping SongPeiping Song1Yahui Yue,Yahui Yue1,2Jing Xie,Jing Xie1,2
  • 1State Key Laboratory of Tibetan Plateau Earth System Science, Resources and Environment (TPESRE), Institute of Tibetan Plateau Research, Chinese Academy of Sciences, Beijing, China
  • 2Center for Excellence in Tibetan Plateau Earth Sciences, Chinese Academy of Sciences, Beijing, China
  • 3University of Chinese Academy of Sciences, Beijing, China
  • 4Department of Earth Sciences, Montana State University, Bozeman, MT, United States
  • 5Department of Geosciences, University of Arizona, Tucson, AZ, United States
  • 6Institute of Science and Technology Strategy, Jiangxi Academy of Sciences, Nanchang, China

A Corrigendum on
New Paleomagnetic Constraints on the Early Cretaceous Paleolatitude of the Lhasa Terrane (Tibet)

by Li Z, Ding L, Laskowski AK, Burke WB, Chen Y, Song P, Yue Y and Xie J (2022). Front. Earth Sci. 10:785726. doi: 10.3389/feart.2022.785726

In the original article, there was a mistake in Table 2 as published. In the “Reference” column, “Combined analysis with results from Li et al. (2016),” the citation should be Li Z. et al. (2017) instead of Li et al. (2016). The corrected Table 2 appears below.

TABLE 2
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TABLE 2. Summary of Cretaceous and Early Cenozoic paleomagnetic poles from the Lhasa and Tethyan-Himalayan (two are from interior of Indian craton) terranes.

In the original article, there was a mistake in Figure 10 as published. The selected reference site appearing in the top-right corner of the figure should read “Reference site (29.5°N, 91.0°E)” instead of “Reference site: 29.7°N, 91.0°E.” The corrected Figure 10 appears below.

FIGURE 10
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FIGURE 10. Paleolatitudes evolution of the Eurasian and Indian continents, the Lhasa terrane, and the Tethyan Himalayan terrane as a function of time. Cretaceous paleomagnetic poles of the Lhasa terrane, which were compiled from previously published results, are listed in Table 2. All paleolatitudes were calculated for the reference site (29.5°N, 91.0°E). Expected paleolatitudes of the Eurasian and Indian continents are drawn from Torsvik et al. (2008, 2012).

In the original article, the reference for Li Z. et al. (2017) was incorrectly written as “Li, Z., Ding, L., Song, P., Fu, J., and Yue, Y. (2017d). Paleomagnetic Constraints on the Paleolatitude of the Lhasa Block during the Early Cretaceous: Implications for the Onset of India-Asia Collision and Latitudinal Shortening Estimates across Tibet and Stable Asia. Gondwana Res. 41, 352–372. doi: 10.1016j.gr.2015.05.013.” Instead, it should be “Li, Z., Ding, L., Song, P., Fu, J., and Yue, Y. (2017). Paleomagnetic Constraints on the Paleolatitude of the Lhasa Block during the Early Cretaceous: Implications for the Onset of India-Asia Collision and Latitudinal Shortening Estimates across Tibet and Stable Asia. Gondwana Res. 41, 352–372. doi: 10.1016/j.gr.2015.05.013.”

In the original article, the reference for Qasim et al. (2018) was not cited. The citation has now been inserted in Section 8 Discussion, “Sub-section 8.2 Implications to Timing of Initial India-Asia Collision,” Paragraph 14:

“Recently, scientists have studied the timing of initial India-Asia collision from the perspectives of biostratigraphic constraints and sedimentary records (DeCelles et al., 2014; Wu et al., 2014; Hu et al., 2015, 2016a; Qasim et al., 2018; Wei et al., 2020).”

In the original article, there was an error in the text. The authors mistakenly wrote “7,100 ± 530 km” and “6,400 ± 550 km” as “7,100 ± 540 km” and “6,400 ± 560 km”. A correction has been made to the Section Highlights, point 3:

“The Neo-Tethys Ocean reached its maximum N-S width of 7,100 ± 530 km at ∼132 Ma and shrank to 6,400 ± 550 km at ∼115 Ma.”

In the original article, there was an error. The authors mistakenly wrote “lower” as “higher.” A correction has been made to Section 5 Magnetic Mineralogy and Petrography, “Sub-section 5.1.2 Temperature Dependence of the Magnetic Susceptibility Measurements,” Paragraph 1:

“Moreover, all samples show that the heating curves are significantly lower than the cooling curves.”

In the original article, there was an error. The authors wrongly cited the reference citation of Li et al. (2016). A correction has been made to Section 8 Discussion, “Sub-section 8.2 Implications to Timing of Initial India-Asia Collision,” Paragraph 12:

“Thus, given the originality of this batch of paleomagnetic data set, it is clear that we also demonstrate the robustness of the previously obtained paleomagnetic results from the Duoni Fm. volcano-sedimentary rocks (Li Z. et al., 2017).”

The authors apologize for these errors and state that this does not change the scientific conclusions of the article in any way. The original article has been updated.

Publisher’s Note

All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.

Reference

Li, Z., Ding, L., Song, P., Fu, J., and Yue, Y. (2017). Paleomagnetic Constraints on the Paleolatitude of the Lhasa Block during the Early Cretaceous: Implications for the Onset of India-Asia Collision and Latitudinal Shortening Estimates across Tibet and Stable Asia. Gondwana Res. 41, 352–372. doi:10.1016/j.gr.2015.05.013

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Keywords: Lhasa terrane, India-Asia collision, Neo-Tethys ocean, paleolatitude, geochronology, intracontinental crustal shortening

Citation: Li Z, Ding L, Laskowski AK, Burke WB, Chen Y, Song P, Yue Y and Xie J (2022) Corrigendum: New Paleomagnetic Constraints on the Early Cretaceous Paleolatitude of the Lhasa Terrane (Tibet). Front. Earth Sci. 10:953708. doi: 10.3389/feart.2022.953708

Received: 26 May 2022; Accepted: 09 June 2022;
Published: 11 July 2022.

Edited and reviewed by:

Derek Keir, University of Southampton, United Kingdom

Copyright © 2022 Li, Ding, Laskowski, Burke, Chen, Song, Yue and Xie. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

*Correspondence: Zhenyu Li, bGl6eUBpdHBjYXMuYWMuY24=

Disclaimer: All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article or claim that may be made by its manufacturer is not guaranteed or endorsed by the publisher.