Re-Entrant Albedo Proton Fluxes Measured by the PAMELA Experiment
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M., Boezio, E. A. Bogomolov, M. Bongi, V. Bonvicini, S. Bottai, A. Bruno, F., Cafagna, D. Campana, P. Carlson, M. Casolino, G. Castellini, C. De Donato, C., De Santis, N. De Simone, V. Di Felice, V. Formato

TL;DR
This paper reports precise measurements of albedo proton fluxes above 70 MeV by the PAMELA experiment, classifying them into different trapped and un-trapped populations and analyzing the penumbra region near the geomagnetic cutoff.
Contribution
It provides a detailed classification and characterization of high-energy albedo protons at low Earth orbit, improving understanding of their populations and behaviors.
Findings
Identification of quasi-trapped and un-trapped proton populations.
Detailed analysis of the penumbra region near the geomagnetic cutoff.
Enhanced characterization of high-energy albedo proton fluxes.
Abstract
We present a precise measurement of downward-going albedo proton fluxes for kinetic energy above 70 MeV performed by the PAMELA experiment at an altitude between 350 and 610 km. On the basis of a trajectory tracing simulation, the analyzed protons were classified into quasi-trapped, concentrating in the magnetic equatorial region, and un-trapped spreading over all latitudes, including both short-lived (precipitating) and long-lived (pseudo-trapped) components. In addition, features of the penumbra region around the geomagnetic cutoff were investigated in detail. PAMELA results significantly improve the characterization of the high energy albedo proton populations at low Earth orbits.
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Astro and Planetary Science · Gamma-ray bursts and supernovae
