Primary Convener: Marine Lasbleis, Université de Nantes, LPG, CNRS, Nantes, France
Conveners: Sarah M Arveson, Yale University, Earth and Planetary Sciences, New Haven, CT, United States, Christopher J Davies, University of Leeds, School of Earth and Environment, Leeds, United Kingdom and Daniel Andrew Frost, University of California Berkeley, Berkeley Seismological Laboratory, Berkeley, CA, United States
Primary Liaison: Marine Lasbleis, ELSI, Tokyo, Japan
Chairs: Marine Lasbleis, ELSI, Tokyo, Japan, Sarah M Arveson, University of California Berkeley, Earth and Planetary Science, Berkeley, CA, United States, Christopher J Davies, Oregon State University, College of Earth, Ocean, and Atmospheric Sciences, Corvallis, United States and Daniel Andrew Frost, Arizona State University, Tempe, AZ, United States
OSPA Liaison: Daniel Andrew Frost, Arizona State University, Tempe, AZ, United States
Numerical Geodynamo Simulations Can Capture the Long-Term Variability of the Paleomagnetic Field (750013)
Domenico G Meduri1, Andrew Biggin2, Christopher J Davies3, Richard K. Bono2 and Courtney Jean Sprain4, (1)University of Liverpool, Department of Earth, Ocean and Ecological Sciences, Liverpool, L69, United Kingdom, (2)University of Liverpool, Department of Earth, Ocean and Ecological Sciences, Liverpool, United Kingdom, (3)University of Leeds, School of Earth and Environment, Leeds, United Kingdom, (4)University of Florida, Department of Geological Sciences, Ft Walton Beach, FL, United States
Strange fields: non-uniformitarian paleomagnetic records imply that the geodynamo process has been substantially perturbed on multiple occasions (734196)
Andrew John Biggin1, Annique van der Boon1, Louise Hawkins2, Daniele Thallner1, Joseph Michael Grappone Jr2, Richard K. Bono3, Domenico G Meduri4, Simon Lloyd2, Ben Handford2, Courtney Jean Sprain5 and Christopher J Davies6, (1)University of Liverpool, Liverpool, L69, United Kingdom, (2)University of Liverpool, Liverpool, United Kingdom, (3)University of Liverpool, Department of Earth, Ocean and Ecological Sciences, Liverpool, United Kingdom, (4)University of Liverpool, Department of Earth, Ocean and Ecological Sciences, Liverpool, L69, United Kingdom, (5)University of Florida, Department of Geological Sciences, Ft Walton Beach, FL, United States, (6)University of Leeds, School of Earth and Environment, Leeds, United Kingdom
Spin transitions and compressibility of ε-Fe7N3 and γ’-Fe4N: implications for iron alloys in terrestrial planetary cores (774105)
Mingda Lv1, Jiachao Liu1, Feng Zhu2, Jie Li2, Dongzhou Zhang3, Yuming Xiao4 and Susannah Dorfman1, (1)Michigan State University, Earth and Environmental Sciences, East Lansing, MI, United States, (2)University of Michigan Ann Arbor, Department of Earth and Environmental Sciences, Ann Arbor, MI, United States, (3)University of Hawaii at Manoa, Hawaii Institute of Geophysics and Planetology, School of Ocean and Earth Science and Technology, Honolulu, HI, United States, (4)Argonne National Laboratory, High Pressure Collaborative Access Team, X-ray Science Division, Argonne, IL, United States