Modeling the acceleration and modulation of anomalous cosmic ray oxygen

Details Modeling the acceleration and modulation of anomalous cosmic ray oxygen Modeling the acceleration and modulation of anomalous cosmic ray oxygen

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011adspr..48...65s&link_type=abstract

Advances in Space Research, Volume 48, Issue 1, p. 65-75.

Physics

1

Scientific paper

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.

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