Fine structure in the gamma-ray sky and the origin of UHECR

@inproceedings{ADErlykin2006FineSI,
  title={Fine structure in the gamma-ray sky and the origin of UHECR},
  author={A.D.Erlykin and A.W.Wolfendale},
  year={2006}
}
The EGRET results for gamma ray intensities in and near the Galactic Plane have been analysed in some detail. Attention has been concentrated on energies above 1 GeV and the individual intensities in a $4^{\circ}$ longitude bin have been determined and compared with the large scale mean found from a nine-degree polynomial fit. Comparison has been made of the observed standard deviation for the ratio of these intensities with that expected from variants of our model. The basic model adopts… Expand