An M6.5-class flare was observed at N12E56 of the solar surface at 16:06 UT on July 8, 2014. In association with this flare, solar neutron detectors located on two high mountains, Mt. Sierra Negra and Chacaltaya and at the space station observed enhancements in the neutral channel. The authors analysed these data and a possible scenario of enhancements produced by high-energy protons and neutrons is proposed, using the data from continuous observation of a solar surface by the ultraviolet telescope onboard the Solar Dynamical Observatory (SDO).
|Número de artículo||050|
|Publicación||Proceedings of Science|
|Estado||Publicada - 2015|
|Evento||34th International Cosmic Ray Conference, ICRC 2015 - The Hague, Países Bajos|
Duración: 30 jul. 2015 → 6 ago. 2015