Fig. 2. Altitude-dependent modeled differential spectra of helium nuclei( He) in anomalous cosmic rays( ACRs), illustrating flux variation with kinetic energy and altitude in Earth ' s stratosphere.
Fig. 3. Modeled altitude-dependent differential spectra of multi-charged oxygen nuclei in anomalous cosmic rays( ACRs), showing flux variation with kinetic energy and altitude in Earth ' s stratosphere.
The surface plot, marked by a color gradient, illustrates the modeled flux intensities across the specified altitudes and energy ranges. The color intensities and surface shapes reflect the distribution and peak densities of ACRs. The model also distinguishes between different charge states of oxygen nuclei, such as O + 1, O + 2, O + 3, and O + 4, representing ionized oxygen. These distinctions are important
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