Primary Convener:
Catherine Constable, University of California San Diego

Convener:
Regupathi Angappan, Johns Hopkins University
Richard Saltus, University of Colorado at Boulder
Daniele Thallner, University of Florida
Alec Brenner, Yale University
Manoj Nair, University of Colorado Boulder
Catherine Johnson, University of British Columbia
Aaron Nielsen, Air Force Institute of Technology

Early Career Convener:
Nicole Clizzie, Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California San Diego

Chair:
Nicole Clizzie, Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California San Diego
Richard Saltus, University of Colorado at Boulder
Daniele Thallner, University of Liverpool

This session will cover a broad range of observations, theoretical developments and numerical simulations of dynamos in Earth and other planets. We solicit contributions covering dynamo simulations, modern field observations, excursions and reversals, and records from deep time and their implications for Earth and planetary evolution. Observations and time series derived from a broad range of materials are both important in their own right and can contribute to global syntheses, continuous time-varying models, and statistical representations of paleosecular variations. Planet-wide modeling and regional records provide important constraints on the temporal evolution of magnetic fields. New modeling strategies for paleomagnetic, direct ground, and satellite observations can offer improved insight and integrations with the products of numerical simulations. We anticipate wide-ranging discussion of all these topics.

Index Terms
1510 Dynamo: theories and simulations
1522 Paleomagnetic secular variation
1532 Reference fields: regional, global
5734 Magnetic fields and magnetism

Cross-Listed:
P - Planetary Sciences
DI - Study of the Earth´s Deep Interior
SM - SPA-Magnetospheric Physics

Neighborhoods:
2. Earth Interior

Co-Organized Sessions:
Study of Earth´s Deep Interior