Het archief bekijken van zondag 21 april 2002
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 2002 Apr 21 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 111 gepubliceerd omstreeks 2200Z op 21 Apr 2002
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 20-2100Z tot 21-2100Z
Solar activity has been high. Region 9906 (S14W90)
produced a long-duration X1/1f flare at 0151 UTC which was
accompanied by strong radio bursts, type II and type IV radio
sweeps, and a partial halo CME. The CME moved extremely rapidly in
the plane of the sky with a projected velocity of 2400-2500 km/s.
The front of the CME appeared to be moving away from the west limb
and therefore approximately perpendicular to the line of sight. The
remainder of today's activity consisted of a few C-class events. A
filament was observed to lift off the northeast part of the disk at
21/0012 UTC and was associated with a narrow CME from the northeast
limb. Region 9912 (N10W12) has continued to grow and is currently
the largest group on the disk now that 9906 has rotated behind west
limb. 9912 was stable and quiet. Two new regions were assigned
today: 9915 (N11E54) and 9916 (S17E71).
IB. Voorspelling zonneactiviteit
Solar activity is expected to be low
to moderate. Region 9906 could contribute an M-class event during
the next 24 hours, but will become less of a threat as it moves
further behind the limb. There is a slight chance for an isolated
M-class event from Region 9912.
IIA. Samenvatting geofysische activiteit 20-2100Z tot 21-2100Z
The geomagnetic field was quiet to unsettled during the past 24
hours. A greater than 100 MeV proton event began at 21/0155 UTC in
response to the X1 flare and continues in progress. The maximum flux
observed so far was 23 PFU at 21/1025 UTC. A greater than 10 MeV
proton event began at 21/0225 UTC and also continues in progress.
The maximum flux at greater than 10 MeV was 2210 PFU at 21/1315 UTC.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is
expected to be quiet to unsettled for most of tomorrow. However, an
increase is expected late on the 22nd due to a glancing blow from
today's partial halo CME. Conditions are expected to attain mostly
active with some minor storm periods at high latitudes. There is a
slight chance, however, for minor to major storm intervals if the
CME should prove to be extraordinarily wide. Conditions should
return to unsettled to active by the 24th. The greater than 10 MeV
proton event should continue for at least 48 hours and the greater
than 100 MeV proton event is expected to continue for the next 12-24
hours.
III. Kans zonnevlammen van 22 Apr tot 24 Apr
Klasse M | 35% | 25% | 20% |
Klasse X | 10% | 05% | 05% |
Proton | 99% | 99% | 20% |
PCAF | in progress
|
IV. Penticton 10.7 cm Flux
Geobserveerd 21 Apr 173
Voorspeld 22 Apr-24 Apr 170/175/180
90 dagen gemiddelde 21 Apr 200
V. Geomagnetische A index
Geobserveerd Afr/Ap 20 Apr 030/062
Geraamd Afr/Ap 21 Apr 007/007
Voorspeld Afr/Ap 22 Apr-24 Apr 015/015-025/030-015/020
VI. Kansen op geomagnetische activiteit van 22 Apr tot 24 Apr
A. Gemiddelde breedtegraad |
Actief | 35% | 45% | 35% |
Kleine storm | 20% | 25% | 20% |
Zware-ernstige stormcondities | 15% | 20% | 15% |
B. Hoge breedtegraad |
Actief | 25% | 30% | 25% |
Kleine storm | 25% | 30% | 25% |
Zware-ernstige stormcondities | 20% | 25% | 20% |
Alle tijden in UTC
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