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Positron decrement in AMS-02 compared to Pamela, due to solar cycle

High Energy Astrophysical Phenomena 2012-11-06 v1
Authors: J. P. Roberts
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Abstract

We present a numerical simulation of cosmic ray transport in the heliosphere and show that AMS-02 should observe a decrease in the positron fraction above 40GeV compared to the fraction observed by PAMELA.

Keywords

cosmic ray transport heliosphere positron fraction ams-02 pamela solar cycle numerical simulation

Cite

@article{arxiv.1211.0691,
  title  = {Positron decrement in AMS-02 compared to Pamela, due to solar cycle},
  author = {J. P. Roberts},
  journal= {arXiv preprint arXiv:1211.0691},
  year   = {2012}
}

Comments

5 pages, 3 figures

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