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xxth GENERAL ASSEMBLY OF IUGG VIENNA (AUSTRIA)

xxth GENERAL ASSEMBLY OF IUGG VIENNA (AUSTRIA)

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GAMl.l<br />

*** CALL FOR PAPERS ***<br />

DIVISION I - INTERNAL MAGNETIC FIELDS<br />

Secular Variation; Modern,<br />

Prehistorical<br />

Jeremy Bloxham, Dept of Earth &<br />

Harvard University, 20 Oxford<br />

MA 02138,USA. [Fax: 617 495 8839]<br />

Stanislav Braginsky<br />

<strong>ASSEMBLY</strong> 1991<br />

Historical and<br />

Planetary<br />

Street,<br />

Sciences,<br />

Cambridge<br />

Topics covered will range f rom studies of the short period<br />

secular variation based on modern observations, through<br />

studies over hundreds of years from historical observations,<br />

to studies spanning tens or hundreds of thousands of years<br />

based on archaemagnetic and palaeomagnetic measurements. The<br />

symposium should provide a developing insight into the<br />

geodynamo.<br />

GAM1.2 Geodynamo Processes and Boundary Conditions<br />

Andrew M Soward, School of Mathematics,<br />

The University, Newcastle upon Tyne NEl 7RU, UK.<br />

David E Loper<br />

Aspects of geodynamo theory will be considered, including core<br />

dynamics but excluding direct numerical simulation which will<br />

be addressed in another session. Conditions at the core-mantle<br />

interface will be considered 1n relation to boundary<br />

conditions for dynamo models, including structure, composition<br />

and dynamics of the D" layer.<br />

GAM1.3 Numerical Modelling of Planetary Dynamos<br />

D R Fearn, Dept of Mathematics, Glasgow University,<br />

University Gardens, Glasgow Gl2 8QW,UK.<br />

K-H Radler<br />

All aspects of numerical modelling of planetary dynamos will<br />

be considered , with particular e mphasis on full<br />

magnetohydrodynamic dynamos.<br />

GAM1.4 Core Waves, Instabilities and Surface Flows<br />

Kathy Whaler, Dept of Earth Sciences, Leeds<br />

University, Leeds LS2 9JT, UK.<br />

Ibrahim A Eltayeb<br />

This session will provide a forum for models of<br />

geomagnetically derived flows at the core surface and their<br />

interpretation . Topics to be covered include waves in the<br />

core , shown by the morphology of the field and the westward<br />

drift, and the initiation, growth and propagation of<br />

instabilities .<br />

19

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