Nonlinear Multi-Scale Processes in the Heliosphere in the IHY

Details Nonlinear Multi-Scale Processes in the Heliosphere in the IHY Nonlinear Multi-Scale Processes in the Heliosphere in the IHY

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....10486c&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #10486

Astronomy and Astrophysics

Astrophysics

Scientific paper

University of Warwick's Space and Astrophysics Group have undertaken an intensive research programme in magnetospheric, heliospheric and solar physics, including analytical theory, large scale numerical simulation, advanced visualization techniques and theory led data analysis. The unifying theme is that these are nonlinear multiscale processes, which control the energy release and conversion processes, turbulence and self-organisation. The coordinated studies of solar, heliospheric and magnetospheric processes proposed in frames of the IHY provide a unique opportunity to unify knowledge that is presently fragmented. For example, remote sensing of physical processes in the solar corona with the use of ground-based and space-borne facilities (potentially, including the multiple vantage point observations with STEREO), remote (e.g. IPS) and in-situ (e.g. WIND, CLUSTER) studies of the development of these processes in the solar wind and the coupling to the dynamic Earth magnetosphere (as indicated by scaling in geomagnetic indices and POLAR UVI images of dynamic auroras) and ionosphere, will allow us to understand the chain of solar-terrestrial connections and, in particular, the nonlinear processes governing these connections.

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