| Issue |
EPJ Web Conf.
Volume 210, 2019
Ultra High Energy Cosmic Rays 2018 (UHECR 2018)
|
|
|---|---|---|
| Article Number | 04005 | |
| Number of page(s) | 6 | |
| Section | Phenomenology | |
| DOI | https://doi.org/10.1051/epjconf/201921004005 | |
| Published online | 17 May 2019 | |
https://doi.org/10.1051/epjconf/201921004005
Progress in the Global Modeling of the Galactic Magnetic Field
1
Institute for Nuclear Physics, Karlsruhe Institute of Technology, Karlsruhe, Germany
2
Center for Cosmology and Particle Physics, New York University, New York, USA
* Michael.Unger@kit.edu
** Glennys.Farrar@nyu.edu
Published online: 17 May 2019
We discuss the global modeling of the properties of the Galactic Magnetic Field (GMF). Several improvements and variations of the model of the GMF from Jansson & Farrar (2012) (JF12) are investigated in an analysis constrained by all-sky rotation measures of extragalactic sources and polarized and unpolarized synchrotron emission data from WMAP and Planck. We present the impact of the investigated model variations on the propagation of ultrahigh-energy cosmic rays in the Galaxy
© The Authors, published by EDP Sciences, 2019
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