Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.kosmofizika.ru/katalog/e05/event2005_06_16.doc Дата изменения: Mon Aug 24 12:35:40 2015 Дата индексирования: Sun Apr 10 23:07:47 2016 Кодировка: koi8-r

Event 2005.06.16- (2005-167)

Particle event: To(Ep>10MeV) - 16d20h
Tmax(Ep>10MeV) - 17d04h, Jmax (Ep>10MeV) - 41
/cm2.s.sr
Duration of the event - 2 days
Energy of the SCR and 0.1 GCR fluxes balance - Eb
= 510 MeV

Sources: ? solar flare 16d20h01m, M4/SF, N09W87, АR10775
Main X-ray burst 1-8 ?: onset - 16d20h01m, max - 16d20h22m, Ф = 0.062 J/m2
CME: gap

Particle fluxes and associated phenomena
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Integral time-of-maximum proton spectrum
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Integral fluxes of protons for the event of 2005.06.16

|S/c, |Eр, |To |Tmax |Jmax, |Dura-t|Comments |
|instruments|MeV | | |(cm2.s.sr)-1 |ion | |
|GOES-10 | | | | | | |
|EPS |>5 |20h |17d04h |57 |2d | |
|EPS |>10 |20h |17d04h |41 |2d | |
|EPS |>30 |20h |17d02h |16 |2d | |
|EPS |>50 |20h |23h |8.7 |2d | |
|EPS |>60 |20h |23h |6.5 |2d | |
|EPS |>100 |20h |23h |2.6 |2d | |
|POES-16 | | | | | | |
|MEPED |>0.24 |20h |- |- |- | |
|MEPED |>0.8 |20h |- |- |- | |
|MEPED |>2.5 |20h |- |- |- | |
|MEPED |>6.9 |20h |23h |110 |2d | |
|MEPED |>16 |20h |23h |36 |2d | |
|MEPED |>36 |20h |23h |25 |2d | |
|MEPED |>70 |20h |23h |4.5 |2d | |
|MEPED |>140 |20h |23h |0.8 |2d | |
|ACE | | | | | | |
|SIS |>10 |20h |17d02h |84.5 |2d | |
|SIS |>30 |20h |17d02h |40 |1d | |
|SOHO | | | | | | |
|EPHIN (INT)|>50 |21h |17d01h |2.8 |1d | |


Differential fluxes of protons for the event of 2005.06.16

|S/c, |?Е, |To |Tmax |Jmax, |Dura-t|Comments |
|instruments|MeV | | |(cm2.s.sr.MeV)|ion | |
| | | | |-1 | | |
|SOHO | | | | | | |
|LION |0.75-2|22h |17d04h |2.3 |3d | |
|LION |2-6 |22h |17d04h |0.9 |3d | |
|EPHIN |4-8 |23h |17d04h |3.5 |3d | |
|EPHIN |8-25 |22h |17d04h |1.4 |2d | |
|EPHIN |25-41 |22h |17d01h |0.3 |2d | |
|EPHIN |41-53 |- " - |- " - |- " - |- " - | |

References:
Mu J., Wang J.S., Zhao H.J., et.al., 2010.
Веселовский И.С., Мягкова И.Н., Яковчук О.С., 2012.



























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