TY  - JOUR
PB  - SciPost Foundation
DO  - 10.21468/SciPostPhysProc.13.001
TI  - Proton penetration efficiency over a high altitude observatory in Mexico
PY  - 2023/09/28
UR  - https://scipost.org/SciPostPhysProc.13.001
JF  - SciPost Physics Proceedings
JA  - SciPost Phys. Proc.
VL  - 
IS  - 13
SP  - 001
A1  - Miyake, S.
AU  - Koi, T.
AU  - Muraki, Yasushi
AU  - Matsubara, Y.
AU  - Masuda, S.
AU  - Miranda, P.
AU  - Naito, T.
AU  - Ortiz, E.
AU  - Oshima, A.
AU  - Sakai, T.
AU  - Sako, T.
AU  - Shibata, S.
AU  - Takamaru, H.
AU  - Tokumaru, M.
AU  - Valdés-Galicia, J. F.
AB  - 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.
ER  -

@Article{10.21468/SciPostPhysProc.13.001,
	title={{Proton penetration efficiency over a high altitude observatory in Mexico}},
	author={S. Miyake and T. Koi and Y. Muraki and Y. Matsubara and S. Masuda and P. Miranda and T. Naito and E. Ortiz and  A. Oshima and T. Sakai and T. Sako and S. Shibata and H. Takamaru and M. Tokumaru and J. F. Valdés-Galicia},
	journal={SciPost Phys. Proc.},
	pages={001},
	year={2023},
	publisher={SciPost},
	doi={10.21468/SciPostPhysProc.13.001},
	url={https://scipost.org/10.21468/SciPostPhysProc.13.001},
}