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Physics of ion acceleration in the solar flare on 2005 September 7 determines γ-ray and neutron production

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Harris,  M. J.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Watanabe, K., Lin, R. P., Krucker, S., Murphy, R. J., Share, G. H., Harris, M. J., Gros, M., Muraki, Y., Sako, T., Matsubara, Y., Sakai, T., Shibata, S., Valdes-Galicia, J. F., González, L. X., Hurtado, A., Musalem, O., Miranda, P., Martinic, N., Ticona, R., Velarde, A., Kakimoto, F., Tsunesada, Y., Tokuno, H., & Ogio, S. (2009). Physics of ion acceleration in the solar flare on 2005 September 7 determines γ-ray and neutron production. Advances in Space Research, 44(7), 789-793. doi:10.1016/j.asr.2009.06.002.


引用: https://hdl.handle.net/11858/00-001M-0000-0011-BF02-3
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