Spectra of Fe ions in powerful SCR events
- Авторлар: Baranov D.G.1, Dergachev V.A.1, Nymmik R.A.2, Panasyuk M.I.2
-
Мекемелер:
- Ioffe Institute
- Skobeltsyn Institute of Nuclear Physics
- Шығарылым: Том 81, № 2 (2017)
- Беттер: 128-131
- Бөлім: Proceedings of the 34th All-Russian Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/184948
- DOI: https://doi.org/10.3103/S1062873817020058
- ID: 184948
Дәйексөз келтіру
Аннотация
Large solar cosmic ray (SCR) events are registered by PLATAN equipment in September–October 1989 aboard the MIR orbital station and in October–November 2003 aboard the International Space Station (ISS). The energy spectra of Fe ions in the energy intervals of 5–200 MeV/nucleon (1989) and 25–90 MeV/nucleon (2003) are measured. Spectra for SCR events of 1989 and 2003 are approximated with high accuracy by the power law function of energy. The SCR events of 1989 greatly exceed those of 2003 in the fluence of Fe particles. High enrichment of the elemental composition of the SCR events 2003 with Fe ions is observed.
Авторлар туралы
D. Baranov
Ioffe Institute
Хат алмасуға жауапты Автор.
Email: d.baranov@bk.ru
Ресей, St. Petersburg, 194021
V. Dergachev
Ioffe Institute
Email: d.baranov@bk.ru
Ресей, St. Petersburg, 194021
R. Nymmik
Skobeltsyn Institute of Nuclear Physics
Email: d.baranov@bk.ru
Ресей, Moscow, 119991
M. Panasyuk
Skobeltsyn Institute of Nuclear Physics
Email: d.baranov@bk.ru
Ресей, Moscow, 119991
Қосымша файлдар
