xxth GENERAL ASSEMBLY OF IUGG VIENNA (AUSTRIA)
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