Contribution of each major CR element in the abundance, ionisation, and destruction when Af/Ai = 0 is considered.
|Element||Abundance||Ionisation||Destruction, for Af/Ai = 0|
|α = 1.0||α = 1.2||α = 1.4|
Notes. The cosmic ray elemental abundances used are those given by GALPROP, at 100 MeV per nucleon, using the “reacceleration model”. The contribution of different CR elements in the destruction, when Af/Ai ≠ 0 is considered, can be seen in Fig. 10.
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