Anti-particles in the inner magnetosphere: energetic positron population

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I. M. Martin
A. A. Gusev
G. I. Pugacheva
M. G. Silva Mello

Resumen

Se analiza la generación de antipartículas atrapadas en el cinturón interior de la magnetosfera. Dichas partículas podrían tener flujos en exceso de los flujos interestelares generados por rayos cósmicos. Al considerar la existencia de un cinturón natural de positrones en la magnetosfera, proponemos que dichos positrones serla generados por una reacción nuclear de los protones relativistas atrapados en el cinturón anterior con la atmosfera residual. El espectro calculado de positrones a 10-100 MeV en el nivel superior L = 1.2 concuerda con los resultados experimentales.

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Martin, I. M., Gusev, A. A., Pugacheva, G. I., & Silva Mello, M. G. (1996). Anti-particles in the inner magnetosphere: energetic positron population. Geofísica Internacional, 35(1), 73–76. https://doi.org/10.22201/igeof.00167169p.1996.35.1.1102
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