scholarly journals Modeling the Galactic Magnetic Field and its Application in verifying a Pulsar Origin of Very High Energy Cosmic Rays

2014 ◽  
Vol 490 ◽  
pp. 012029 ◽  
Author(s):  
Pantea Davoudifar ◽  
Keihanak Rowshan Tabari
Keyword(s):  
Magnetic Field ◽  
Cosmic Rays ◽  
High Energy ◽  
Galactic Magnetic Field ◽  
High Energy Cosmic Rays ◽  
Very High Energy ◽  
Very High

scholarly journals Propagation of Ultra-high-energy Cosmic Rays in Galactic Magnetic Field

2011 ◽  
Author(s):  
Hajime Takami ◽  
Hiroyuki Sagawa ◽  
Yoshiya Kawasaki ◽  
Takashi Sako ◽  
Masahiro Takeda ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Cosmic Rays ◽  
High Energy ◽  
Ultra High Energy ◽  
Galactic Magnetic Field ◽  
High Energy Cosmic Rays

Very High-Energy Cosmic Rays

1963 ◽  
Vol 11 (4) ◽  
pp. 172-173 ◽  
Author(s):  
C. E. Fichtel
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
High Energy Cosmic Rays ◽  
Very High Energy ◽  
Very High

scholarly journals The KASCADE-Grande observatory and the composition of very high-energy cosmic rays

2015 ◽  
Vol 651 ◽  
pp. 012001 ◽  
Author(s):  
J C Arteaga-Velázquez ◽  
W D Apel ◽  
K Bekk ◽  
M Bertaina ◽  
J Blümer ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
High Energy Cosmic Rays ◽  
Very High Energy ◽  
Very High

scholarly journals Origins of Extragalactic Cosmic Ray Nuclei by Contracting Alignment Patterns induced in the Galactic Magnetic Field

2019 ◽  
Vol 210 ◽  
pp. 04004
Author(s):  
Martin Erdmann ◽  
Lukas Geiger ◽  
David Schmidt ◽  
Martin Urban ◽  
Marcus Wirtz
Keyword(s):  
Magnetic Field ◽  
Cosmic Rays ◽  
Cosmic Ray ◽  
High Energy ◽  
Ultra High Energy ◽  
Galactic Magnetic Field ◽  
High Energy Cosmic Rays ◽  
Novel Approach ◽  
Astrophysical Scenario ◽  
The Individual

We present a novel approach to search for origins of ultra-high energy cosmic rays. In a simultaneous fit to all observed cosmic rays we use the galactic magnetic field as a mass spectrometer and adapt the nuclear charges such that their extragalactic arrival directions are concentrated in as few directions as possible. During the fit the nuclear charges are constraint by the individual energy and shower depth measurements. We show in a simulated astrophysical scenario that source directions can be reconstructed even within a substantial isotropic background.

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