GP21A:
Refining Our Understanding of Earth and Planetary Magnetic Processes with Accurate Paleointensity Estimates II Posters


Submit an Abstract to this Session


Session ID#: 45491

Session Description:
Accurately obtaining the strength of paleomagnetic fields (paleointensity) from Earth and extraterrestrial bodies is a key objective for studying many Earth and planetary processes, such as the thermal evolution of the core of Earth and planets, the formation and evolution of the early solar system, the formation and crystallization of the inner core and the possibility of an upcoming geomagnetic field reversal. This session welcomes contributions, which present high-quality absolute or relative paleointensity estimates that allow us to better understand Earth and planetary magnetic processes. We especially welcome contributions that develop new experimental techniques and analytical approaches to help us better estimate paleointensities. We also welcome (but not limited to) rock magnetic, microscopic and petrological studies that aid us to obtain accurate paleointensities, especially dealing with thermal alteration and multidomain effects for absolute paleointensities, and normalization issues for relative paleointensities.
Primary Convener:  Huapei Wang, China University of Geosciences (Wuhan), School of Geophysics and Geomatics, Wuhan, China
Conveners:  Greig A Paterson, University of Liverpool, School of Environmental Sciences, Liverpool, United Kingdom and Joseph Michael Grappone Jr, University of Liverpool, Liverpool, United Kingdom
Primary Liaison:  Huapei Wang, China University of Geosciences (Wuhan), School of Geophysics and Geomatics, Wuhan, China
Chairs:  Greig A Paterson1, Joseph Michael Grappone Jr1 and Huapei Wang2, (1)University of Liverpool, Liverpool, United Kingdom(2)China University of Geoscences (Wuhan), Wuhan, China
OSPA Liaison:  Greig A Paterson, University of Liverpool, Liverpool, United Kingdom
Index Terms:

1521 Paleointensity [GEOMAGNETISM AND PALEOMAGNETISM]
1527 Paleomagnetism applied to geologic processes [GEOMAGNETISM AND PALEOMAGNETISM]
1540 Rock and mineral magnetism [GEOMAGNETISM AND PALEOMAGNETISM]
1595 Planetary magnetism: all frequencies and wavelengths [GEOMAGNETISM AND PALEOMAGNETISM]

Abstracts Submitted to this Session:

Shelby Anne Jones, Scripps Institution of Oceanography, La Jolla, CA, United States, Arielle Thibeault, University of California San Diego, Scripps Institution of Oceanography, La Jolla, CA, United States, Eric Blinman, New Mexico Office of Archaeological Studies (OAS), Santa Fe, United States, Jeff Royce Cox, New Mexico Department of Cultural Affairs, New Mexico Office of Archaeological Studies, Santa Fe, NM, United States, Stacey N Lengyel, East Tennessee State University, Johnson City, TN, United States and Lisa Tauxe, Scripps Institution of Oceanography, University of California San Diego, La Jolla, United States
Joseph Michael Grappone Jr, University of Liverpool, Liverpool, United Kingdom, John Shaw, Univ Liverpool, Liverpool, United Kingdom, Andrew John Biggin, University of Liverpool, Department of Earth, Ocean and Ecological Sciences, Liverpool, United Kingdom and Mimi J Hill, University of Liverpool, Liverpool, L69, United Kingdom
Hoabin Hong1, Liao Chang1 and Akira Hayashida2, (1)Peking University, School of Earth and Space Sciences, Beijing, China, (2)Faculty of Science and Engineering, Doshisha University, Kyotanabe, Japan
Marine Séverine Foucher, Michigan Technological University, Geological and Mining Engineering and Sciences, Houghton, MI, United States, Katie E Bristol, Michigan Technological University, Geological and Mining Engineering and Sciences, Houghton, United States, Elisa J Piispa, University of Iceland, Institute of Earth Sciences, Reykjavik, Iceland and Aleksey V Smirnov, Michigan Technological University, Department of Geological and Mining Engineering and Sciences, Houghton, United States
Huapei Wang, China University of Geosciences (Wuhan), School of Geophysics and Geomatics, Wuhan, China, Dennis V Kent, Lamont -Doherty Earth Observatory of Columbia University, Paleomagnetics Lab, Palisades, United States; Lamont-Doherty Earth Observatory of Columbia University, Palisades, United States and Huafeng Qin, State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
Greig A Paterson, University of Liverpool, School of Environmental Sciences, Liverpool, United Kingdom, Adrian R Muxworthy, Imperial College London, Earth Science and Engineering, London, United Kingdom, Yuhji Yamamoto, Kochi University, Center for Advanced Marine Core Research, Kochi, Japan, Yongxin Pan, Paleomagnetism and Geochronology Laboratory, Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China and Katie King, University of Southampton, Southampton, United Kingdom
Hanna Fethee Asefaw1, Lesleis Nagy2, Lisa Tauxe2 and Wyn Williams3, (1)Scripps Institution of Oceanography, La Jolla, CA, United States, (2)Scripps Institution of Oceanography, University of California San Diego, La Jolla, United States, (3)Univ Edinburgh, Edinburgh, United Kingdom