Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.kosmofizika.ru/katalog/e98/event1998_11_24.doc Дата изменения: Mon Aug 24 12:40:02 2015 Дата индексирования: Sun Apr 10 23:08:30 2016 Кодировка: koi8-r

Event 1998.11.24 - (1998-328)

Particle event: To(Ep>10 MeV) - 24d03h
Tmax(Ep>10 MeV) - 24d10h, Jmax (Ep>10 MeV) - 1.25
/cm2.s.sr *)
Duration of the event - 2 days *)
Energy of the SCR and 0.1 GCR fluxes balance - Eb
= 210 MeV
*) According to data IMP-8 (CPME)

Sources: ? solar flare 24d02h07m, X1.0/SF, S30W81, AR8384
Main x-ray burst 1-8 ?: onset - 24d02h07m, max - 24d02h20m, Ф = 0.12 J/m2
CME: 24d02h30m, V = 1798 km/s, ?? = 360?, dA = 225?

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 1998 November 24

|IMP-8 | | | | | | |
|CPME |1-2 |05h |10h |1.2 |- | |
|CPME |2-4.6 |05h |10h |0.5 |- | |
|CPME |4.6-15 |05h |10h |0.1 |- | |
|CPME |15-25 |05h |10h |0.04 |2d | |
|CPME |25-48 |05h |10h |0.01 |2d | |
|CPME |48-96 |05h |10h |0.0035 |2d | |
|CPME |96-145 |05h |10h |0.002 |1d | |
|CPME |145-440 |05h |10h |0.001 |1d | |
|SOHO | | | | | | |
|LION |0,75-2 |02h |10h |0.6 |6d | |
|LION |2-6 |02h |10h |0.12 |6d | |
|EPHIN |4-8 |03h |09h |0.31 |5d | |
|EPHIN |8-25 |03h |09h |0.07 |4d | |
|EPHIN |25-41 |03h |09h |0.015 |2d | |
|EPHIN |41-53 |- " - |- " - |- " - |- " - | |

References
Hoshida T., Y. Matsubara, Y. Muraki et al. (in all 70 authors of Tibet
Collaboration). A possible observation of solar neutrons in association
with November 28th, 1998 flare. - Proc. 26th Int. Cosmic Ray Conf., Salt
Lake City, USA, 1999, v.6, p.38-41.
23 ноября с амплитудой сигнала of 3.4? Тибетский нейтронный телескоп
отметил сигнал от вспышечных нейтронов. Протоны ™10 МэВ начали приходить к
Земле около 03:00 UT и достигли максимума около 10:00 UT.
.

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