CaltechAUTHORS
  A Caltech Library Service

Characterizing the Geomagnetic Field at High Southern Latitudes: Evidence From the Antarctic Peninsula

Biasi, Joseph and Kirschvink, Joseph L. and Fu, Roger R. (2021) Characterizing the Geomagnetic Field at High Southern Latitudes: Evidence From the Antarctic Peninsula. Journal of Geophysical Research. Solid Earth, 126 (12). Art. No. e2021JB023273. ISSN 2169-9313. doi:10.1029/2021jb023273. https://resolver.caltech.edu/CaltechAUTHORS:20220107-513223500

[img] PDF - Accepted Version
See Usage Policy.

2MB
[img] PDF - Supplemental Material
See Usage Policy.

13MB
[img] PDF - Supplemental Material
See Usage Policy.

253kB
[img] MS Excel (Table S1) - Supplemental Material
See Usage Policy.

27kB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20220107-513223500

Abstract

Due to a dearth of data from high-latitude paleomagnetic sites, it is not currently clear if the geocentric axial dipole (GAD) hypothesis accurately describes the long-term behavior of the geomagnetic field at high latitudes. Here we present new paleomagnetic and paleointensity data from the James Ross Island (JRI) volcanic group, located on the Antarctic Peninsula. This data set addresses a notable lack of data from the 60°–70°S latitude bin and includes 251 samples from 31 sites, spanning 0.99–6.8 Ma in age. We also include positive fold, conglomerate, and baked contact tests. Paleointensity data from three methods (Thellier-Thellier, pseudo-Thellier, and Tsunakawa-Shaw) were collected from all sites. The Thellier-Thellier method had low yields and produced unreliable data, likely due to sample alteration during heating. Results from the Tsunakawa-Shaw and pseudo-Thellier methods were more consistent, and we found a bimodal distribution of paleointensity estimates. Most sites yielded either <15 μT or >40 μT, which together span a range of estimates from long-term geomagnetic field models, but do not favor any model in particular. Alternating-field demagnetization of these samples, when combined with preexisting data, yields a revised paleomagnetic pole of −87.5°, 025°, α95 = 3.6° for the Antarctic Peninsula over the last ∼5 Ma, which suggests that the current data set is sufficiently large to “average out” secular variation. Finally, the C2r/C2n transition was probably found at a site on JRI, and further geochronological and paleomagnetic study of these units could refine the age of this reversal.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1029/2021jb023273DOIArticle
https://earthref.org/MagIC/19313Related ItemPaleomagnetic data
ORCID:
AuthorORCID
Biasi, Joseph0000-0003-1196-7877
Kirschvink, Joseph L.0000-0001-9486-6689
Fu, Roger R.0000-0003-3635-2676
Additional Information:© 2021. American Geophysical Union. Issue Online: 24 December 2021; Version of Record online: 24 December 2021; Accepted manuscript online: 14 December 2021; Manuscript accepted: 11 December 2021; Manuscript revised: 09 December 2021; Manuscript received: 18 September 2021. The authors would like to thank their fellow team members: Jennifer Buz, David Flannery, Ross Mitchell, Joe O’Rourke, Steve Skinner, Sarah Slotznick, David Smith, Frank Sousa, and Tom Tobin for their patience and assistance with sample collection. The authors also thank the crew of the Nathaniel B. Palmer and Air Center Helicopters for their logistical support. This work was funded by NSF Polar Programs grant ANT-1341729 to J. L. Kirschvink and an NSF EAR Postdoctoral Fellowship grant (2052963) to J. Biasi. The authors are not aware of any conflicts of interest that would affect this manuscript. Data Availability Statement: Tables S1–S10 in Supporting Information S2, which contain sample metadata, pole summaries, least-squares fits, paleointensity selection criteria, paleointensity results, and VGPs from previous studies, are available with the online version of this manuscript. A supplementary file containing additional descriptions of field locations, field photos, rock magnetics figures, demagnetization plots, and paleointensity figures is also available online. All paleomagnetic data are available via the MagIC database at https://earthref.org/MagIC/19313.
Funders:
Funding AgencyGrant Number
NSFANT-1341729
NSFEAR-2052963
Subject Keywords:James Ross Island; paleomagnetism; paleointensity; Antarctica; volcanology; tangent cylinder
Issue or Number:12
DOI:10.1029/2021jb023273
Record Number:CaltechAUTHORS:20220107-522574800
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20220107-513223500
Official Citation:Biasi, J., Kirschvink, J. L., & Fu, R. R. (2021). Characterizing the geomagnetic field at high southern latitudes: Evidence from the Antarctic Peninsula. Journal of Geophysical Research: Solid Earth, 126, e2021JB023273. https://doi.org/10.1029/2021JB023273
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:112785
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:09 Jan 2022 21:08
Last Modified:09 Jan 2022 21:08

Repository Staff Only: item control page