Fig. 6.From: The interaction between the Moon and the solar windThe hybrid model magnetic field magnitude [nT] along y at x = −6.5 Rl = −11245 km for two different upstream solar wind conditions (labeled before and after), compared to WIND observations from Ogilvie et al. (figure 1, 1996). The vertical lines show the location of the optical shadow, and the x-axis shows time on December 27, 1994, as in the original plot.Back to article page