Galactic Structure and the Cosmic Ray Anisotropy at 10¹⁸eV

R. W. Clay

Abstract

Received 2000 November 16, accepted 2001 March 15

Cosmic ray arrival directions at energies a little over 10¹⁸ eV have been reported to show an excess from directions close to that of the Galactic centre. That result was originally presented by the AGASA group and was later strengthened by an analysis of SUGAR cosmic ray data. We discuss here a second feature of the AGASA data, a deficit in roughly the Galactic anticentre direction.We interpret this as a result of cosmic ray diffusion past us. We find that the most straightforward interpretation of the data then requires that a strong magnetic field exists out of the plane of our Galaxy to distances of at least several kiloparsecs.

Keywords: cosmic rays — ISM: magnetic fields

Publications of the Astronomical Society of Australia 18(2) 148 - 150 (2001) doi:10.1071/AS01032