Het archief bekijken van woensdag 7 januari 2004
Activiteitenrapport
Bij elke genoemde zonnevlam in dit rapport werd een schaalfactor toegepast door het Space Weather Prediction Center (SWPC). Vanwege de SWPC-schaalfactor worden zonnevlammen 42% kleiner gerapporteerd dan voor de wetenschappelijke data. De schaalfactor werd verwijderd uit onze gearchiveerde zonnevlamdata om de werkelijke fysieke eenheden weer te geven.
Rapport van de zonne- en geofysische activiteit van 2004 Jan 07 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 007 gepubliceerd omstreeks 2200Z op 07 Jan 2004
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 06-2100Z tot 07-2100Z
Solar activity was high. An M4 x-ray event occurred at
0404 UTC and an M8 x-ray event occurred at 1027 UTC. Both events
were from Region 537 (N07E64) and were associated with type II
sweeps and CMEs off the east limb. The region rotated more fully
into view today as a small (280 millionths) but bright and
magnetically complex sunspot group. Region 536 (S11W02) continues to
be the largest group on the disk and is maintaining its
beta-gamma-delta configuration. There was some indication today that
the region may be slowly decaying. Region 536 could only manage to
produce a couple B-class events. Two new, small, simple regions
emerged on the disk today: Region 538 (N07E04) and Region 539
(N09E29).
IB. Voorspelling zonneactiviteit
Solar activity is expected to be
moderate with a chance for isolated major flare activity. Region 537
is expected to remain active and Region 536 still has the potential
for producing significant flare activity as well.
IIA. Samenvatting geofysische activiteit 06-2100Z tot 07-2100Z
The geomagnetic field ranged from unsettled to major storm levels
during the past 24 hours. An enhancement in the solar wind flow was
observed at ACE, beginning 2000 UTC on 06 January. The enhancement
consisted of an increase in total field and in solar wind velocity,
and included some extended negative Bz intervals in the -1 to -10 nT
range. Although the flow was somewhat atypical (low density, high
temperature), the signatures appear to be consistent with a CME led
by a compression wave and expanding in low density solar wind that
originated in association with the M6 x-ray event on 5 January. The
slow rotation of Bz from negative to positive during the last 18
hours resulted in a decrease in geomagnetic activity during the last
5-6 hours of the period. The greater than 2 MeV electron fluxes were
high during the past 24 hours.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is
expected to be mostly active with some minor storm periods for 08
January based on the continued influence of a high speed solar wind
stream. Mostly active conditions should predominate on 09 January
and a decline to mostly unsettled levels is expected on 10 January.
III. Kans zonnevlammen van 08 Jan tot 10 Jan
Klasse M | 65% | 65% | 65% |
Klasse X | 15% | 15% | 15% |
Proton | 05% | 05% | 05% |
PCAF | green
|
IV. Penticton 10.7 cm Flux
Geobserveerd 07 Jan 119
Voorspeld 08 Jan-10 Jan 120/125/125
90 dagen gemiddelde 07 Jan 135
V. Geomagnetische A index
Geobserveerd Afr/Ap 06 Jan 017/020
Geraamd Afr/Ap 07 Jan 030/030
Voorspeld Afr/Ap 08 Jan-10 Jan 025/030-020/020-015/015
VI. Kansen op geomagnetische activiteit van 08 Jan tot 10 Jan
A. Gemiddelde breedtegraad |
Actief | 35% | 30% | 25% |
Kleine storm | 25% | 20% | 15% |
Zware-ernstige stormcondities | 15% | 10% | 05% |
B. Hoge breedtegraad |
Actief | 15% | 25% | 25% |
Kleine storm | 50% | 35% | 25% |
Zware-ernstige stormcondities | 25% | 20% | 15% |
Alle tijden in UTC
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