Paleointensity extremes: Dynamic implications and future fields

Lead Research Organisation: University of Liverpool
Department Name: Earth, Ocean and Ecological Sciences

Abstract

I propose to use my recently developed modeling techniques to resolve a fundamental disconnect between measurements of the strength of the ancient geomagnetic field (paleointensity) and theories of Earth's core dynamic and use this to answer outstanding questions about how fast Earth's magnetic field can change and how our protective barrier might change in the foreseeable future.

Earth's magnetic field has been protecting our planet for at least 3.4 billion years and, despite being one on the oldest known features of Earth, there remain many aspects of how the field is generated and how it has evolved over time that are poorly understood. This makes is difficult to predict how the field will behave in the future. Currently, our best predications of future variations only extend about 5 years into the future. This is often too short to meet the needs of long terms investments, such as those required for space satellites and ground based power infrastructure, which rely on the shielding provided by the magnetic field.

To predict future changes in the geomagnetic field we have to unravel past changes in the field and the physics that governs them. Understanding the evolution of the deep Earth and the physics behind extreme geomagnetic features, such as rapid field changes, are frontiers in paleomagnetic research that have implications for the predictability of our protective barriers future. However, our ability to understand these phenomena is held back by the uncertain reliability of the paleointensity data needed to understand these key features. To push these boundaries forward, we must ensure the fidelity of our observations, which requires a full understanding of the physical behavior that affects paleointensity data. This is especially important for time periods where the observed paleointensities contradict our most advanced understanding of how the magnetic field works.

This project will use my newly developed tools to bridge the gap between specimen-level paleointensity data and global geomagnetic field reconstructions, and will take a radically different approach that utilizes "big data" analyses of millions of simulated and real results. Much like a surveyor would assess a building based on the quality of the materials and how they were used to construct the building, I will assess the building blocks of paleointensity data to determine the quality of the results.

Armed with this new capability, I will provide a robust assessment of the validity of the Levantine archeomagnetic spikes, which record field intensity changes with rates tens faster than ever observed. Such extreme changes are beyond current dynamo theory and their resolution may have a profound impact on how we understand the dynamics of the outer core. Then, using a next generation geomagnetic field construction spanning the last 4,000 years, I will determine the longevity of the recent decline in dipole field strength and assess how long into the near future the current weakening of Earth's magnetic shield is likely to persist and how it will affect the modern world and the technologies that we all rely on in our daily lives.

Planned Impact

The proposed project is broadly "blue skies" in nature and the immediate benefactors will be the Earth science community. In particular, those studying geomagnetic field dynamics and evolution, deep Earth interior processes, and paleointensity methods. However, the ability to achieve more accurate and longer-term forecasts of geomagnetic variations has important societal and economic benefits. Many aspects of modern technology are sensitive to the effects of solar wind radiation that our magnetic field shields against and predictions of variability decades into the future are invaluable to governments and industries seeking to invest in long term projects such as power infrastructure as well as scientific and communication satellites.

This project will establish a robust records of extreme paleomagnetic field variability during the last ~4,000 years, which will have significant impact on current geodynamo theories. Ensuring that the geomagnetic modeling community obtains the maximum benefit from this work will aid their ability to predict the future variability of Earth's magnetic field. A special session at the 2021 AGU Fall meeting, in addition to a domestic UK workshop, will be organized to maximize engagement with the academic beneficiaries. These will ensure the widest attendance by people engaged in all areas of magnetic research and key speakers will be invited to bring together all potential users. General dissemination of project results and information on the uses of magnetism in Earth sciences will be achieved through the Geomagnetism.org website.

A further advantage of the Geomagnetism.org website is the ease with which a wider audience can interact with it. This will provide a medium to engage the general public with the aim of increasing society's appreciation for Earth sciences and science in general. I will participate in NERC training for communicating science to the public, which will be undertaken early in the project so that techniques learned may be immediately implemented to maximize the non-academic impact of the project. These skills will be used to communicate the ideas and benefits of science to the public through university open days, web articles, and other opportunities that may arise during the fellowship.

I will also participate in the Royal Society's MP-Scientist Pairing Scheme. This scheme will allow me to directly communicate the importance of paleomagnetic research in terms of providing constraints on the future geomagnetic field that are necessary to make informed decisions about future investments in key technology and fundamental infrastructure.

The close collaboration with international researchers will be beneficial to the reputation of British science. My extensive experiences working in China will also strengthening Sino-British relations. There are many scientific opportunities in the rapidly developing Chinese scientific community and researchers there are keen to cultivate new international collaborations and expand the impact of their work and the development of Chinese science. This also gives rise to potential opportunities for student exchanges. My reintegration back into British science following several years in China will improve cultural awareness in the UK and will broaden the general public's appreciation of a science as a multinational endeavor.

Publications

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Chevrier DM (2023) Collective magnetotaxis of microbial holobionts is optimized by the three-dimensional organization and magnetic properties of ectosymbionts. in Proceedings of the National Academy of Sciences of the United States of America

 
Description Particles to Planets: Unravelling the history of our magnetic field
Amount £649,335 (GBP)
Funding ID NE/W006707/1 
Organisation Natural Environment Research Council 
Sector Public
Country United Kingdom
Start 10/2022 
End 10/2025
 
Description School Geophysics
Amount £2,415 (GBP)
Organisation Royal Astronomical Society 
Sector Academic/University
Country United Kingdom
Start 05/2020 
End 05/2021
 
Title Paleointensity.org: an online, open source, application for the interpretation of paleointensity data - source codes 
Description First release of the paleointensity.org python codes for archiving on Zenodo Paleointensity.org is an online, open source, application to analyze paleointensity data produced by the most common paleointensity techniques. Our application currently supports four different methods: thermal Thellier (all variations), microwave Thellier, pseudo-Thellier and the multispecimen protocol. Data can be imported using a variety of input file formats such as ThellierTool files, the generic PmagPy file format, and a number of lab-specific formats. The data for the individual paleointensity methods is visualized by the relevant graphs and parameters, which are updated dynamically while interpreting the data. Beyond manual interpretation, Paleointensity.org features an auto-interpreter for specimen level Thellier-type data. Interpretations and data can be exported to csv and MagIC files. Moreover, it is possible to export the local storage containing all data, saved interpretations, and settings. This file can be shared among researchers or attached to a paper as supplementary information. Because of its many features and ease of use, Paleointensity.org is a major step forward in enhancing an open paleomagnetic community in which data can be shared, checked, and reused in line with the FAIR (Findable, Accessible, Interoperable, and Reusable) data principles. 
Type Of Material Database/Collection of data 
Year Produced 2020 
Provided To Others? Yes  
Impact The publication associated with this piece of software currently has 10 citations. 
URL https://zenodo.org/record/3744224
 
Title The PINT absolute palaeointensity database 
Description The aim of the PINT database is to catalogue all absolute palaeointensity data with ages > 50 ka which have been published in the peer-reviewed literature. 
Type Of Material Database/Collection of data 
Year Produced 2022 
Provided To Others? Yes  
Impact The publication of this database has led to the development of a follow on publication. The database has a growing global users with over 450 unique users within its first 12 month period. 
URL http://pintdb.org/
 
Title greigpaterson/Magnetic_to_the_Core_Survey: First Release 
Description The first release of the data 
Type Of Material Database/Collection of data 
Year Produced 2022 
Provided To Others? Yes  
Impact This repository contains the supplementary data for van der Boon et al. (2022). The data are responses to a survey quiz given to attendees of the Royal Society Summer Science Exhibition in 2019. Supplement file 1 contains the quiz questions and supplement file 2 contains the responses. van der Boon, A., Biggin, A. J., Paterson, G. A., Kavanagh, J. L. (2022). Magnetic to the Core - communicating palaeomagnetism with hands-on activities, Geosci. Commun., doi: 10.5194/gc-2021-41). 
URL https://zenodo.org/record/6257839
 
Title HystLab 
Description HystLab is MATLAB based software for advanced processing and analysis of magnetic hysteresis loop data. HystLab is an easy to use graphical interface that is compatible with a wide range of software platforms and data formats. 
Type Of Technology Software 
Year Produced 2018 
Open Source License? Yes  
Impact No standardized approach or software existed in the Earth science magnetics community to process and analyze magnetic hysteresis loop data, one of the mostly widely used magnetic measurements. HystLab, and its associated publication (Paterson et al., 2018, doi: 10.1029/2018GC007620), filled this void, giving users advanced tools in an easy-to-use software package. The software has received wide praise when presented at the 16th Castle Meeting, 2018, Poland, and the AGU Fall 2018 meeting, USA. 
URL http://dx.doi.org/10.1029/2018GC007620
 
Title paleointensity.org 
Description paleointensity.org is an online web application for the analysis of paleointensity data (data pertaining to the strength of the geomagnetic field). A major novelty of this site is the ability to analyses multiple methods in a single application - something that was not previously possible in any other software. The web application is FAIR (Findable, Accessible, Interoperable, Reusable) data compliant and offers compatibility with a wide range of standard and custom data formats, as well as though used by community databases. 
Type Of Technology Webtool/Application 
Year Produced 2020 
Open Source License? Yes  
Impact The recent development of this software tool means that information on its impact is currently unavailable. 
URL https://paleointensity.org/
 
Description Ness Botanic Gardens Family Science Fair 
Form Of Engagement Activity Participation in an activity, workshop or similar
Part Of Official Scheme? No
Geographic Reach Local
Primary Audience Public/other audiences
Results and Impact We presented a new developed rock or choc game and Earth Science related coloring picture at Ness Botanical Gardens as part of their annual Family Science Fair. More than 100 members of the public (predominantly families with children) attended. This helped us to hone and refine our activities for future events.
Year(s) Of Engagement Activity 2019
 
Description Royal Society Summer Science Exhibition 2019 
Form Of Engagement Activity Participation in an activity, workshop or similar
Part Of Official Scheme? No
Geographic Reach National
Primary Audience Public/other audiences
Results and Impact The Geomagnetism Group at the University of Liverpool hosted a stand entitled "Magnetic to the Core" at the 2019 Royal Society Summer Science Exhibition. We exhibited activities related to our Earth Science Magnetism research to ~12,600 visitors, which included > 1,500 school students. The results of a questionnaire revealed a statistically significant increase in knowledge of Earth magnetism of attendees that had visited our stand for at least 10 minutes versus attendees who had not visited our stand.
Year(s) Of Engagement Activity 2019
URL https://royalsociety.org/science-events-and-lectures/2019/summer-science-exhibition/exhibits/
 
Description School Geophysics Lunch Club 
Form Of Engagement Activity Participation in an activity, workshop or similar
Part Of Official Scheme? No
Geographic Reach Local
Primary Audience Schools
Results and Impact A weekly lunch time geophysics club at Scarrisbrick Hall School, Lancashire, where Year 11-12 pupils and learn about geophysics and undertake geophysical survey and experiments (e.g., ground penetrating radar surveys, or performing paleomagnetic experiments). Initially started as a one-off event, interested in geophysics has grown and this is now a regular event.
Year(s) Of Engagement Activity 2021,2022,2023
 
Description University of Liverpool Year 6 STEM event 
Form Of Engagement Activity Participation in an open day or visit at my research institution
Part Of Official Scheme? No
Geographic Reach Regional
Primary Audience Schools
Results and Impact Faculty organized STEM event for ~80 Year 6 pupils. We presented a range of activities around magnetic materials to introduce pupils Earth Science magnetism. Teachers were interested in how to incorporate some of our concepts and information into their their own lessons.
Year(s) Of Engagement Activity 2022
 
Description Victoria Gallery & Museum School Holiday Workshop 
Form Of Engagement Activity Participation in an activity, workshop or similar
Part Of Official Scheme? No
Geographic Reach Local
Primary Audience Schools
Results and Impact We presented four fun activities (a selfie shoot; rock magnetometer; a magnetic globe; and a rock or choc game) at a University of Liverpool housed Victoria Gallery & Museum as part of their annual School Holiday activity day. Around 30-50 school children and their parents attended.This served as trial run for our Royal Society event.
Year(s) Of Engagement Activity 2019