Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.izmiran.rssi.ru/~ichertok/SEPs_radio/fig4s.htm
Дата изменения: Fri Mar 23 03:38:19 2012 Дата индексирования: Sun Apr 10 01:19:18 2016 Кодировка: Windows-1251 Поисковые слова: ацобс бфмбофйюеулбс бопнбмйс |
Distribution
of the analyzed SEPs with different >100 MeV proton fluxes (J100) at the microwave
flux density plane 'S9 vs. S15'. The following points deserve attention:
(1) General
correspondence takes place between intensities of microwave bursts and proton
fluxes - J100 increases when S9 and S15
rise.
(2) Among
events with relatively weak radio fluxes (S9, S15
<1000 sfu), weak proton fluxes (J100<1
pfu) under soft radio spectra (S9>S15)
dominate.
(3)
Powerful microwave bursts (S9, S15>3000-10000
sfu) with hard radio spectra (S9<S15)
correspond to majority of powerful proton fluxes (J100 >10
pfu).
(4) SEPs with moderate proton fluxes rank intermediate positions.