- #1
vaart
- 7
- 0
Dear All,
I have a question regarding the understanding of anisotropy of cosmic rays and how to understand them better. To determine the anisotropy I have seen a lot of papers where they use maps that have a Relative Intensity map and a Statistical significance map of the sky.
I understand the relative intensity map, but I don't understand why the statistical significance maps are used, could some one explain this to me?
Thanks,
caart
I have a question regarding the understanding of anisotropy of cosmic rays and how to understand them better. To determine the anisotropy I have seen a lot of papers where they use maps that have a Relative Intensity map and a Statistical significance map of the sky.
I understand the relative intensity map, but I don't understand why the statistical significance maps are used, could some one explain this to me?
Thanks,
caart