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Observation of the Forbush decrease on 2024 May 10, using the ALPAQUITA air-shower array at the 70-1000 GV rigidity range

Fuente: arXiv

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Bibliographic Details
Main Authors:	Anzorena, M., de la Fuente, E., Fujita, K., Garcia, R., Hayashi, Y., Hibino, K., Hotta, N., Imaizumi, G., Katayose, Y., Kato, C., Kato, S., Kawashima, T., Kawata, K., Kobayashi, M., Kobayashi, S., Koi, T., Kojima, H., Miranda, P., Mitsuishi, S., Mizuno, A., Munakata, K., Nakamura, Y., Nishizawa, M., Noguchi, Y., Ogio, S., Ohishi, M., Ohnishi, M., Oshima, A., Raljevic, M., Rivera, H., Saito, T., Sako, T., Sako, T. K., Shibata, S., Shiomi, A., Subieta, M., Sugimoto, F., Tajima, N., Takano, W., Takeyama, Y., Takita, M., Tamaki, N., Tameda, Y., Tanaka, K., Ticona, R., Tsuchiya, H., Tsunesada, Y., Udo, S., Yamagishi, G., Yamanaka, Y., Yamazaki, K., Yokoe, Y.
Format:	Preprint
Published:	2026
Subjects:	High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2601.08154