Fig. 1.From: Magnetic shadowing of high energy ions at Mars and how this effect can be simulated using a hybrid modelEnhanced particle fluxes recorded by SLED in Channels 3 and 6 during March, 1989 in association with major ongoing flaring. Significant depressions in flux due to magnetic shadowing are indicated by dashed vertical lines. Following McKenna-Lawlor et al. (1991).Back to article page