Proton Penetration Efficiency over a High Altitude Observatory in Mexico

Miyake, S.
Koi, T.
Muraki, Y.
Matsubara, Y.
Masuda, S.
Miranda, P.
Naito, T.
Ortiz, E.
Oshima, A.
Sakai, T.
Sako, T.
Shibata, S.
Takamaru, H.
Tokumaru, M.
Valdes-Galicia, J. F.

In association with the large solar flare on November 7, 2004, detectors at in Mt. Chacaltaya in Bolivia and Mt. Sierra Negra in Mexico recorded a event. For this explanation, we performed calculations to solve the equation of motion of antiprotons in the magnetosphere. As a result, the Mt. Chacaltaya event and Mt. Sierra Negra event could be explained.

21st International Symposium on Very High Energy Cosmic Ray Intercations

online

10.48550/arXiv.2207.01817

arXiv:2207.01817

Inquiry of Nature Ⅰ

The Natural Sciences Ⅰ