Figures and Tables

From the following article:

Solar wind dynamic pressure and electric field as the main factors controlling Saturn's aurorae

F. J. Crary, J. T. Clarke, M. K. Dougherty, P. G. Hanlon, K. C. Hansen, J. T. Steinberg, B. L. Barraclough, A. J. Coates, J.-C. Gérard, D. Grodent, W. S. Kurth, D. G. Mitchell, A. M. Rymer and D. T. Young

Nature 433, 720-722(17 February 2005)

doi:10.1038/nature03333

BACK TO ARTICLE
Figure 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 1

Solar wind conditions measured by Cassini.

Full size figure and legend (81K)
Figure 2 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 2

Comparison between HST images and solar wind conditions propagated to Saturn for the period 25–30 January 2004.

Full size figure and legend (59K)
Figure 3 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 3

Correlation between HST-derived auroral input power and solar wind conditions.

Full size figure and legend (41K)
BACK TO ARTICLE