Het archief bekijken van maandag 1 november 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 Nov 01 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 306 gepubliceerd omstreeks 2200Z op 01 Nov 2004
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 31-2100Z tot 01-2100Z
Solar activity was moderate. Region 691 (N13W55)
produced today's only M-class flare: an M1/1f at 0322 UTC. The event
was associated with a type II sweep and a relatively slow CME off
the west limb (plane-of-sky speed ~ 500-550 km/s). Region 691 showed
steady decay during the past 24 hours. The most spectacular event of
the period was a bright CME from a source behind the west limb,
which was first observed in the LASCO C2 coronagraph at 0606 UTC.
The absence of disk signatures and observations in EIT 195 imagery
clearly indicate a backside source. The plane-of-sky speed of the
CME was about 800 km/s. Region 693 (S16E08) grew considerably during
the period and is the dominant region on the disk. Although the
group shows occasional brightenings it still has not produced any
flare activity. New Region 696 (N09E63) was assigned today as a
small, D-type group.
IB. Voorspelling zonneactiviteit
Solar activity is expected to be
moderate, but there is a continued slight chance for major flares or
proton producing flares from 691 or 693.
IIA. Samenvatting geofysische activiteit 31-2100Z tot 01-2100Z
The geomagnetic field was quiet to unsettled during the past 24
hours. The arrival of transient flow from the solar events of 30
October has not yet been observed in the solar wind data. Proton
events at greater than 10 MeV and greater than 100 MeV were
observed. The 10 MeV event began at 0655 UTC, reached a maximum of
63 PFU at 0805 UTC, and appears to have ended as of 1900 UTC. The
100 MeV event began at 0635 UTC, reached a maximum of 1.5 PFU at
0645 UTC, and ended at 0755 UTC. The event was well associated with
the backside CME reported in part IA.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is
expected to be predominantly active for the next 24 hours (02
November) as the impact from the solar events of 30 October is still
expected. Conditions should decline to unsettled to slightly active
for 03 November, and should be predominantly unsettled by 04
November.
III. Kans zonnevlammen van 02 Nov tot 04 Nov
Klasse M | 50% | 50% | 50% |
Klasse X | 15% | 15% | 15% |
Proton | 15% | 15% | 15% |
PCAF | yellow
|
IV. Penticton 10.7 cm Flux
Geobserveerd 01 Nov 136
Voorspeld 02 Nov-04 Nov 135/135/130
90 dagen gemiddelde 01 Nov 107
V. Geomagnetische A index
Geobserveerd Afr/Ap 31 Oct 007/010
Geraamd Afr/Ap 01 Nov 012/015
Voorspeld Afr/Ap 02 Nov-04 Nov 020/025-015/015-010/010
VI. Kansen op geomagnetische activiteit van 02 Nov tot 04 Nov
A. Gemiddelde breedtegraad |
Actief | 30% | 25% | 20% |
Kleine storm | 25% | 20% | 15% |
Zware-ernstige stormcondities | 15% | 10% | 05% |
B. Hoge breedtegraad |
Actief | 35% | 30% | 25% |
Kleine storm | 30% | 25% | 20% |
Zware-ernstige stormcondities | 20% | 10% | 05% |
Alle tijden in UTC
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