Abstract
The results of continuous monitoring of the intensity variations of relativistic electron flux (1.5–3 MeV and 3–6 MeV) in the outer radiation belt of the Earth which was done by the MKL instrument onboard the CORONAS-F satellite are presented. The main purpose of the work is analysis of the dynamics of relativistic electron flux in the outer radiation belt of the Earth in particular long increasing of their intensity 10 and more days after magnetic storms.
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Kuznetsov, S.N. et al. (2014). Dynamics of the Relativistic Electrons Flux of the Earth Outer Radiation Belt Based on the MKL Instrument Data. In: Kuznetsov, V. (eds) The Coronas-F Space Mission. Astrophysics and Space Science Library, vol 400. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-39268-9_11
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DOI: https://doi.org/10.1007/978-3-642-39268-9_11
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