In Situ Data and Effect Correlation During September 2017 Solar Particle Event

Solar energetic particles are one of the main sources of particle radiation seen in space. In the first part of September 2017 the most active solar period of cycle 24 produced four large X‐class flares and a series of (interplanetary) coronal mass ejections, which gave rise to radiation storms seen...

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Veröffentlicht in:	Space Weather 2019-01, Vol.17 (1), p.99-117
Hauptverfasser:	Jiggens, P., Clavie, C., Evans, H., O'Brien, T. P., Witasse, O., Mishev, A. L., Nieminen, P., Daly, E., Kalegaev, V., Vlasova, N., Borisov, S., Benck, S., Poivey, C., Cyamukungu, M., Mazur, J., Heynderickx, D., Sandberg, I., Berger, T., Usoskin, I. G., Paassilta, M., Vainio, R., Straube, U., Müller, D., Sánchez‐Cano, B., Hassler, D., Praks, J., Niemelä, P., Leppinen, H., Punkkinen, A., Aminalragia‐Giamini, S., Nagatsuma, T.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aircraft components Avionics Computer simulation Coronal mass ejection Data processing Datasets dose Energetic particles Fluence GLE Heliosphere International Space Station Mars Mars surface Monitors Radiation Radiation detectors Satellite technology Satellites SEEs SEP Single Event Effects Solar corona Solar energetic particles Solar radiation shielding Solar storms Space stations Spacecraft Spacecraft shielding SPE Storms
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