Progress in the Global Modeling of the Galactic Magnetic Field
arXiv:1901.04720 · doi:10.1051/epjconf/201921004005
Abstract
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.
To appear in the proceedings of UHECR18
References in corpus (13)
- A New Electron Density Model for Estimation of Pulsar and FRB Distances
- The Vertical Structure of Warm Ionised Gas in the Milky Way
- Global cosmic-ray related luminosity and energy budget of the Milky Way
- Constraining the Milky Way's Hot Gas Halo with OVII and OVII Emission Lines
- The Vertical Structure of the Outer Milky Way HI Disk
- Rotation Measures of Extragalactic Sources Behind the Southern Galactic Plane: New Insights into the Large-Scale Magnetic Field of the Inner Milky Way
- Pulsar Rotation Measures and Large-scale Magnetic Field Reversals in the Galactic Disk
- The Milky Way Rotation Curve and its Vertical Derivatives Inside the Solar Circle
- Magnetic Fields in a Sample of Nearby Spiral Galaxies
- The Galactic Magnetic Field and Ultrahigh-Energy Cosmic Ray Deflections
- Does the stellar distribution flare? A comparison of stellar scale heights with LAB HI data
- The Nuclear Window to the Extragalactic Universe
- Constraining the vertical structure of the Milky Way rotation by microlensing in a finite-width global disk model
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- What can be learnt from UHECR anisotropies observations Paper II: intermediate-scale anisotropies
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