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

<table>ACS count rate over entire period encompassing the three ICME events studied together with solar wind field and plasma components from ACE and electron strahl from Wind. Highlighted regions indicate presence of flux ropes.</table>

Advances in Astronomy

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Figure 9

Figure 9: Diffusion Coefficients, Short-Term Cosmic Ray Modulation, and Convected Magnetic Structures 