Diffusion Coefficients, Short-Term Cosmic Ray Modulation, and Convected Magnetic Structures

<table>Wind and ACE IMF, plasma, and electron strahl (165 eV) data for 04-13 through 04-14 2006. INTEGRAL ACS data (unshifted) is shown in the bottom panel. The leading and trailing boundaries of the ICME are shown by vertical lines.</table>

Advances in Astronomy

fig8

Figure 8

Figure 8: Diffusion Coefficients, Short-Term Cosmic Ray Modulation, and Convected Magnetic Structures 