Het archief bekijken van maandag 3 november 2003
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 2003 Nov 03 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 307 gepubliceerd omstreeks 2200Z op 03 Nov 2003
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 02-2100Z tot 03-2100Z
Solar activity has been at high levels. Two X-class
events made way for yet another day of impressive major flare
activity. Region 488 (N08W82) produced an X3/2f flare at 03/0955Z
and an X2/2b event at 03/0130Z. Both flares had associated
Tenflares, Type II and IV radio sweeps, and CME's. The associated
CME with the X3 event didn't appear to be Earth directed, though the
X2 event may become slightly geoeffective. This Region has shown
some decay over the period although it remains a very magnetically
complex region with delta structures still evident throughout the
spot cluster. Region 486 (S17W75) was limited in flare production
today. The largest flare from this region was an M3/sf that
occurred at 03/1532Z. This region continues to exhibit a very
complex magnetic field and continues to depict a beta-gamma-delta
magnetic class structure. No new regions were numbered today.
IB. Voorspelling zonneactiviteit
Solar activity is expected to be at
high levels through day one. Regions 486 and 488 are due to exit
the disk beginning on day two which should significantly drop flare
activity by day three of the period.
IIA. Samenvatting geofysische activiteit 02-2100Z tot 03-2100Z
The geomagnetic field was at quiet to active levels. The greater
than 10 MeV proton event that began at 02/1105Z has thus far had a
maximum of 1570 pfu, which occurred at 03/0815Z and has recently
been ranging between 400 and 800 pfu's at the time of this writing.
The greater than 100 MeV proton event began at 02/1740Z, reached a
maximum of 49 pfu at 02/1905Z, and ended at 03/1720Z. The polar cap
absorption event remains in progress. The greater than 2 MeV
electron fluxes at geosynchronous orbit reached high levels today.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is
expected to range from quiet to severe storm levels through day one
of the period. A full halo CME resulting from the X8/2b event from
yesterday is expected to arrive early in the period on day one.
Additional data from SOHO/LASCO imagery indicates that there was
significant deceleration of the CME. Predominantly active
conditions are expected on day two with isolated minor storm levels
expected. Day three should see a return to unsettled to active
levels. The greater than 10 MeV proton event should drop below
alert levels by day two.
III. Kans zonnevlammen van 04 Nov tot 06 Nov
Klasse M | 90% | 90% | 70% |
Klasse X | 75% | 75% | 50% |
Proton | 99% | 75% | 50% |
PCAF | in progress
|
IV. Penticton 10.7 cm Flux
Geobserveerd 03 Nov 167
Voorspeld 04 Nov-06 Nov 145/130/120
90 dagen gemiddelde 03 Nov 131
V. Geomagnetische A index
Geobserveerd Afr/Ap 02 Nov 011/018
Geraamd Afr/Ap 03 Nov 012/015
Voorspeld Afr/Ap 04 Nov-06 Nov 080/090-025/035-015/020
VI. Kansen op geomagnetische activiteit van 04 Nov tot 06 Nov
A. Gemiddelde breedtegraad |
Actief | 25% | 40% | 30% |
Kleine storm | 40% | 35% | 15% |
Zware-ernstige stormcondities | 35% | 15% | 10% |
B. Hoge breedtegraad |
Actief | 10% | 30% | 40% |
Kleine storm | 50% | 45% | 20% |
Zware-ernstige stormcondities | 40% | 20% | 15% |
Alle tijden in UTC
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