2020MNRAS.493.1960A


Query : 2020MNRAS.493.1960A

2020MNRAS.493.1960A - Mon. Not. R. Astron. Soc., 493, 1960-1981 (2020/April-1)

The contribution of nearby supernova remnants on the cosmic ray flux at Earth.

AL-ZETOUN A. and ACHTERBERG A.

Abstract (from CDS):

We consider anisotropic diffusion of Galactic cosmic rays in the Galactic magnetic field, using the Jansson-Farrar model for the field. In this paper, we investigate the influence of source position on the cosmic ray flux at the Earth in two ways: (1) by considering the contribution from cosmic ray sources located in different intervals in Galactocentric radius, and (2) by considering the contribution from a number of specific and individual close-by supernova remnants. Our calculation is performed by using a fully three-dimensional stochastic method. This method is based on the numerical solution of a set of stochastic differential equations, equivalent to Ito formulation, that describes the propagation of the Galactic cosmic rays.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): diffusion - magnetic fields - methods: numerical - cosmic rays - ISM: supernova remnants

Simbad objects: 11

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Number of rows : 11
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SNR G119.5+10.2 SNR 00 06.6 +72 47           ~ 268 1
2 SNR G160.8+02.6 SNR 05 01 00.000 +46 40 00.00           ~ 233 0
3 SNR G180.0-01.7 SNR 05 39 00.000 +27 50 00.00           ~ 294 2
4 NAME Vela SNR 08 34.0 -45 50           ~ 1331 2
5 SNR G299.2-02.9 SNR 12 15 13 -65 30.0           ~ 58 0
6 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
7 SNR G065.2+05.7 SNR 19 33.0 +31 10           ~ 105 0
8 SNR G073.9+00.9 SNR 20 14 15 +36 12.0           ~ 74 0
9 SNR G089.0+04.7 SNR 20 45.0 +50 35           ~ 237 0
10 NAME Cyg Loop SNR 20 51.0 +30 40           ~ 964 0
11 SNR G114.3+00.3 SNR 23 37 05.780 +61 51 01.69           ~ 130 1

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