- To determine in-situ, the properties and dynamics of plasma, fields and
particles in the near-Sun heliosphere.
- To investigate the fine-scale structure and dynamics of the Sun's
magnetised atmosphere, using close-up, high-resolution remote sensing.
- To identify the links between activity on the Sun's surface and the
resulting evolution of the corona and inner heliosphere, using solar
co-rotation passes.
- To observe the polar regions of the Sun (rotation, radiance, magnetic
field, fast wind, and coronal holes) and the equatorial corona from high
latitudes.
|
+44 (0)1483 204100 - Copyright © 1999-2005 UCL