Measurement of the re-entrant all-electron spectrum by the High-Energy Particle Detector on board the China Seismo-Electromagnetic Satellite

Interactions of primary cosmic rays with residual atmospheric nuclei produce secondary leptons through the decay chain of short-lived pions. Even though generated with an upward direction, a fraction of these secondary electrons and positrons is bent back downward towards the Earth by the geomagnetic field lines (hence they are called re-entrant albedo). In this paper, we report on a new measurement of the re-entrant all-electron differential flux in the energy range 10-100 MeV, performed by the High-Energy Particle Detector (HEPD-01) on board the China Seismo-Electromagnetic Satellite (CSES-01) in the near-equatorial region at about 500 km altitude between 2018 and 2022. This analysis focuses on the re-entrant all-electron spectrum that covers the low energy interval in a geographical region characterized by a substantial lack of recent experimental data and can contribute to a more accurate definition of secondary electron and positron population distribution and refine the radiation models in the Earth's magnetosphere.

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Publication Details

Journal
Astroparticle Physics
Published
2025-09-01
DOI
https://doi.org/10.1016/j.astropartphys.2025.103170
Primary Topic
Earthquake Detection and Analysis
Type
article
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Measurement of the re-entrant all-electron spectrum by the High-Energy Particle Detector on board the China Seismo-Electromagnetic Satellite

Simona Zoffoli, G. Osteria, S. Ricciarini, V. Scotti et al.
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Astroparticle Physics
Earthquake Detection and Analysis
article

Measurement of the re-entrant all-electron spectrum by the High-Energy Particle Detector on board the China Seismo-Electromagnetic Satellite

Simona Zoffoli, G. Osteria, S. Ricciarini, V. Scotti, D. Campana, R. Battiston, A. Oliva, M. Sorbara, Z. Sahnoun, C. Neubüser, S. Amoroso, F. Perfetto, Alessandro Sotgiu, M. Martucci, A. Contin, Umberto Savino, F. Nozzoli, Alessio Perinelli, Veronica Vilona, Giuseppe Gebbia, Marco Mese, М. Мерге, M. Lolli, M. Ricci, M. Pozzato, Leonardo Ricci, Silvia Pietroni, Riccardo Nicolaidis, P. Cipollone, B. Panico, A. Lega, C. De Santis, L. Conti, C. De Donato, S. Bartocci, R. Sparvoli, P. Zuccon, P. Picozza, P. Ubertini, W.J. Burger, Francesco Palma, R. Iuppa, S. Beolè, M. Cristoforetti, F. M. Follega, M. V. Suresh Babu, E. Ricci, G. Masciantonio, A. Di Luca
article en

Abstract

Interactions of primary cosmic rays with residual atmospheric nuclei produce secondary leptons through the decay chain of short-lived pions. Even though generated with an upward direction, a fraction of these secondary electrons and positrons is bent back downward towards the Earth by the geomagnetic field lines (hence they are called re-entrant albedo). In this paper, we report on a new measurement of the re-entrant all-electron differential flux in the energy range 10-100 MeV, performed by the High-Energy Particle Detector (HEPD-01) on board the China Seismo-Electromagnetic Satellite (CSES-01) in the near-equatorial region at about 500 km altitude between 2018 and 2022. This analysis focuses on the re-entrant all-electron spectrum that covers the low energy interval in a geographical region characterized by a substantial lack of recent experimental data and can contribute to a more accurate definition of secondary electron and positron population distribution and refine the radiation models in the Earth's magnetosphere.

Astroparticle PhysicsVol. 175
Openalex Percentile: Top 76%
Earthquake Detection and Analysis
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