Отправить статью по E-mail Relationship between the Longitude Distribution of the Heliospheric Characteristics and the GCR Intensity in 2007–2008 and 2014–2015
- Авторы: Krainev M.B.1, Bazilevskaya G.A.1, Borkut I.K.2, Mayorov A.G.2
-
Учреждения:
- Lebedev Physical Institute
- National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
- Выпуск: Том 81, № 9 (2018)
- Страницы: 1355-1361
- Раздел: Interaction of Plasma, Particle Beams, and Radiation with Matter
- URL: https://journals.rcsi.science/1063-7788/article/view/193875
- DOI: https://doi.org/10.1134/S1063778818090156
- ID: 193875
Цитировать
Открытый доступ
Доступ предоставлен
Только для подписчиков
Аннотация
On the basis of the temporal behavior of the galactic cosmic rays and the heliospheric factors observed in 2007–2008 and 2014–2015, their average heliolongitude distributions are formed and compared. In addition to the neutron monitor data, the provisional database of daily average galactic cosmic ray proton intensities measured by the PAMELA satellite-borne experiment in 2006–2015 is used. It is shown that the properties of the heliolongitude distributions in the above periods are substantially different.
Ключевые слова
Об авторах
M. Krainev
Lebedev Physical Institute
Автор, ответственный за переписку.
Email: mkrainev46@mail.ru
Россия, Moscow, 119991
G. Bazilevskaya
Lebedev Physical Institute
Email: mkrainev46@mail.ru
Россия, Moscow, 119991
I. Borkut
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: mkrainev46@mail.ru
Россия, Moscow, 115409
A. Mayorov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: mkrainev46@mail.ru
Россия, Moscow, 115409
Дополнительные файлы
