Modeling the acceleration and modulation of anomalous cosmic ray oxygen
Abstract
After the solar wind termination shock crossings of the Voyager spacecraft, the acceleration of anomalous cosmic rays has become a very contentious subject. In this paper we examine several topics pertinent to anomalous cosmic ray oxygen acceleration and transport using a numerical cosmic ray modulation model. These include the effects of drifts on a purely Fermi I accelerated spectra, the effects of introducing higher charge states of oxygen into the modulation model, examining the viability of momentum diffusion as a re-acceleration process in the heliosheath and examining energy spectra, and intensity gradients, in the inner heliosphere during consecutive drift cycles
URI
http://hdl.handle.net/10394/6989https://doi.org/10.1016/j.asr.2011.03.014
http://www.sciencedirect.com/science/article/pii/S027311771100175X