Forbush Decreases in the Fluxes of Galactic Cosmic Rays, According to the PAMELA Experiment
- 作者: Lagoida I.A.1, Voronov S.A.1, Mikhailov V.V.1
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隶属关系:
- National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
- 期: 卷 83, 编号 8 (2019)
- 页面: 971-973
- 栏目: Article
- URL: https://journals.rcsi.science/1062-8738/article/view/187490
- DOI: https://doi.org/10.3103/S1062873819080252
- ID: 187490
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详细
Amplitudes of Forbush decreases registered in the PAMELA experiment from 2006 to 2014 were analyzed, depending on such characteristics of interplanetary space as the magnitude of the magnetic field modulus, the solar wind velocity, and the plasma temperature. The PAMELA telescope consists of a time-of-flight system, a magnetic spectrometer, anticoincidence systems, an electromagnetic calorimeter, and a neutron detector. It was launched into Earth orbit aboard the Resurs DK1 satellite in June 2006 and continued to work for 10 years.
作者简介
I. Lagoida
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
编辑信件的主要联系方式.
Email: iliyalagoida@gmail.com
俄罗斯联邦, Moscow, 115409
S. Voronov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: iliyalagoida@gmail.com
俄罗斯联邦, Moscow, 115409
V. Mikhailov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: iliyalagoida@gmail.com
俄罗斯联邦, Moscow, 115409
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