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Spatial distributions of electrons with the energy 300-600 keV
[Overview] [2004] [2005] [2006]Spatial distributions of electrons with the energy 300-600 keV measured onboard CORONAS-F (2004-2005 years) and тАЬUniversitetsky-TatyanaтАЭ (2005-2006 years) satellites.
Spatial distributions (geographical map) of trapped, quasi-trapped and precipitated electrons with the energy 300-600 keV measured on board CORONAS-F satellite in evening-night MLT sectors.
| 2004 | September, 1-30 | October, 1-31 | November, 1-30 | December, 1-31 | |
| 2005 | February, 1-28 | March, 1-31 | April, 1-15 | April, 16-30 | June, 1-24 |
Spatial distributions (geographical map) of trapped, quasi-trapped and precipitated electrons with the energy 300-600 keV measured onboard тАЬUniversitetsky-TatyanaтАЭ satellite in evening-night MLT sectors.
| 2005 | March, 1-31 | April, 1-30 | May, 1-31 | June, 1-30 | August, 1- 31 | September, 1-30 | |
| 2006 | January, 1-31 | February, 1-28 | March, 1-31 | April, 1-30 | May, 1-31 | June, 1-30 | July, 1-31 |
Presented maps demonstrate the areas of trapped ( the outer ERB at high latitudes), quasitrapped ( L=2-2.5) and precipitated (L<2 ) electron flux.
2004
Coronas-F
 August |
 September |
 October |
 November |
 December |
2005
Coronas-F
 February |
 March |
 April I |
 April II |
 June |
Universitetsky-Tatyana
 March |
 April |
 May |
 June |
 July |
 August |
 September |
2006
Universitetsky-Tatyana
 January |
 February |
 March |
 April |
 May |
 June |
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