Proton penetration efficiency over a high altitude observatory in Mexico-Reference-Cited by-同舟云学术

Proton penetration efficiency over a high altitude observatory in Mexico

Published:2023-09-28 Issue:13 Volume: Page:
ISSN:2666-4003
Container-title:SciPost Physics Proceedings
language:
Short-container-title:SciPost Phys. Proc.

Author:

Miyake S.¹,Koi T.²,Muraki Yasushi³,Matsubara Y.³,Masuda S.³,Miranda P.⁴,Naito T.⁵,Ortiz E.⁶,Oshima A.²,Sakai T.⁷,Sako T.⁸,Shibata S.²,Takamaru H.²,Tokumaru M.³,Valdés-Galicia J. F.⁶

Affiliation:

1. National Institute of Technology, Kagoshima College

2. Chubu University

3. Nagoya University

4. Higher University of San Andrés

5. University of Yamanashi

6. National Autonomous University of Mexico

7. Nihon University

8. Institute for Cosmic Ray Research

Abstract

In association with a large solar flare on November 7, 2004, the solar neutron detectors located at Mt. Chacaltaya (5,250 m) in Bolivia and Mt. Sierra Negra (4,600 m) in Mexico recorded very interesting events. In order to explain these events, we have performed a calculation solving the equation of motion of anti-protons inside the magnetosphere. Based on these results, the Mt. Chacaltaya event may be explained by the detection of solar neutrons, while the Mt. Sierra Negra event may be explained by the first detection of very high energy solar neutron decay protons (SNDPs) around 6 GeV.

Publisher

Stichting SciPost

Subject

General Medicine

Link

https://scipost.org/10.21468/SciPostPhysProc.13.001/pdf

Reference9 articles.

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