The trajectories of cosmic rays at the highest energies. II. Sensitivity of the anisotropy predictions to model parameters
A Dudarewicz; A A Ivanov; M A Pravdin; X Chi; L Zhang; A W Wolfendale; A Dudarewicz; Dept. of Phys., Durham Univ., UK; A A Ivanov; Dept. of Phys., Durham Univ., UK; M A Pravdin; Dept. of Phys., Durham Univ., UK; X Chi; Dept. of Phys., Durham Univ., UK; L Zhang; Dept. of Phys., Durham Univ., UK; A W Wolfendale; Dept. of Phys., Durham Univ., UK
Журнал:
Journal of Physics G: Nuclear and Particle Physics
Дата:
1994-04-01
Аннотация:
Further numerical calculations of the trajectories of cosmic-ray protons above 10<sup>17</sup> eV have been made following our earlier work. The sensitivity of the derived anisotropies to the parameters of the magnetic field and the nature of the source distribution has been examined. A comparison has been made with the results of other workers.
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