Chapter

The Coronas-F Space Mission

Volume 400 of the series Astrophysics and Space Science Library pp 327-336

Date:

Dynamics of the Relativistic Electrons Flux of the Earth Outer Radiation Belt Based on the MKL Instrument Data

  • S. N. KuznetsovAffiliated withD.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University (SINP MSU) 
  • , I. N. MyagkovaAffiliated withD.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University (SINP MSU) Email author 
  • , E. A. MuravievaAffiliated withD.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University (SINP MSU)
  • , B. Yu. YushkovAffiliated withD.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University (SINP MSU)
  • , L. I. StarostinAffiliated withD.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University (SINP MSU) 
  • , Yu. I. DenisovAffiliated withD.V. Skobeltsyn Institute of Nuclear Physics, M.V. Lomonosov Moscow State University (SINP MSU) 
  • , K. KudelaAffiliated withInstitute of Experimental Physics, Slovak Academy of Sciences (IEP SAS)
 Deceased

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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.