Advances in Astronomy / 2015 / Article / Fig 7

Research Article

Influence of the Atmospheric Mass on the High Energy Cosmic Ray Muons during a Solar Cycle

Figure 7

(a) The annual values of the barometric coefficient for Riyadh and the sunspot number (SSN) for the period 2002 to 2012. (b) is the same as (a) but for Adelaide muon detector for the period 2003 to 2012.

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