Het archief bekijken van maandag 20 mei 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 May 20 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 140 gepubliceerd omstreeks 2200Z op 20 May 2002
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 19-2100Z tot 20-2100Z
Solar activity was high. Region 9961 (S22E62) produced
two M-class flares and one X-class flare during the past 24 hours.
The X-flare was an X2/2n at 1527 UTC and was impulsive. Nonetheless
this flare was associated with a narrow-width CME from the southeast
limb. The first M-flare was an M4 at 1029 UTC and the second was an
M5 at 1053 UTC. Both of these events were impulsive and were
attributed to 9961 based on SOHO/EIT data. Region 9961 appears to be
a compact, magnetically complex group which has at least a gamma
classification, and possibly a magnetic delta. Region 9957 (N09E22)
continues to be the largest group on the disk and has a delta
configuration in a compact collection of spots. A partial halo CME
was observed in C2 at 19/2026 UTC and was centered over the
southwest limb. EIT images at the same time confirmed a front-side
source from the southwest part of the disk.
IB. Voorspelling zonneactiviteit
Solar activity is expected to be
mostly moderate, but there is a chance for an additional major flare
event from either of Region 9961 or 9957.
IIA. Samenvatting geofysische activiteit 19-2100Z tot 20-2100Z
The geomagnetic field was mostly quiet to unsettled during the past
24 hours. There was an isolated active period from 1500-1800 UTC. An
interval of enhanced solar wind flow passed the ACE solar wind
spacecraft beginning at 0257 UTC and lasted about 10 hours. The Bz
magnetic field component was mostly negative with typical values
between -5 nT and -10 nT. The onset of the this flow at Earth caused
a sudden impulse at 0342 UTC, which measured 22 nT on the Boulder
magnetometer.
IIB. Voorspelling geofysische activiteit
The geomagnetic field should be
mostly unsettled tomorrow and quiet to unsettled on the second day.
Activity on the third day is expected increase slightly to unsettled
with some isolated active periods due to possible effects from
today's partial halo CME that began at 19/2026 UTC.
III. Kans zonnevlammen van 21 May tot 23 May
Klasse M | 80% | 80% | 80% |
Klasse X | 20% | 20% | 20% |
Proton | 15% | 15% | 15% |
PCAF | green
|
IV. Penticton 10.7 cm Flux
Geobserveerd 20 May 171
Voorspeld 21 May-23 May 170/170/165
90 dagen gemiddelde 20 May 184
V. Geomagnetische A index
Geobserveerd Afr/Ap 19 May 008/018
Geraamd Afr/Ap 20 May 010/015
Voorspeld Afr/Ap 21 May-23 May 008/010-005/008-012/015
VI. Kansen op geomagnetische activiteit van 21 May tot 23 May
A. Gemiddelde breedtegraad |
Actief | 20% | 20% | 25% |
Kleine storm | 10% | 10% | 15% |
Zware-ernstige stormcondities | 05% | 05% | 10% |
B. Hoge breedtegraad |
Actief | 20% | 20% | 25% |
Kleine storm | 10% | 10% | 20% |
Zware-ernstige stormcondities | 05% | 05% | 15% |
Alle tijden in UTC
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