The overall flux of the cosmic rays measured at the top of the atmosphere is often plotted as sho...
The overall flux of the cosmic rays measured at the top of the atmosphere is often plotted as shown in the figure below. The flux is multiplied by the energy factor E and plotted in double- logarithmic scale. This allows one to emphasise different spectral regions denoted by:I, II, III and IV. Discuss the present understanding of the origin and characteristics of these four regions 2.7 III IV 15 19 log E(ev) 112]
The overall flux of the cosmic rays measured at the top of the atmosphere is often plotted as shown in the figure below. The flux is multiplied by the energy factor E and plotted in double- logarithmic scale. This allows one to emphasise different spectral regions denoted by:I, II, III and IV. Discuss the present understanding of the origin and characteristics of these four regions 2.7 III IV 15 19 log E(ev) 112]