<B>Acceleration, Ionization, and Transport of 
                   Multiply Charged Anomalous Cosmic Rays: 
                   Interpretation of SAMPEX Observations

</B>
<PRE>A.F. Barghouty<sup>1</sup>, J.R. Jokipii<sup>2</sup>, and R.A. Mewaldt<sup>1</sup>
<sup>1</sup>California Institute of Technology
<sup>2</sup>University of Arizona</PRE>
                   Observations by SAMPEX have shown that the ionic charge 
                   state composition of anomalous cosmic rays (ACRs) 
                   is more complex than was previously realized. 
                   At energies &lt25 MeV/nucleon observed 
                   ACR N, O, and Ne are predominantly singly-charged, 
                   but at higher energies they are predominantly 
		   multiply charged.  These observations 
                   place constraints on models for the acceleration 
                   of ACRs at the termination shock as well as their 
                   transport to 1 AU. 
                   We present new simulations of the acceleration, 
                   ionization, and transport of ACR elements He through 
                   Ar, taking advantage of new, theoretically-derived 
                   ionization cross sections. Comparisons to SAMPEX 
                   measurements and implications for models of ACR 
                   acceleration and transport will be presented.