Het archief bekijken van dinsdag 18 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 18 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 322 gepubliceerd omstreeks 2200Z op 18 Nov 2003
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 17-2100Z tot 18-2100Z
Solar activity was at moderate levels again today.
Region 501 (N03E09) produced several M-class flares today. A pair
of M3/2n flares were the most notable, peak fluxes were at 18/0752Z
and 18/0831Z. A filament channel to the south and west of this
region erupted following the first flare. Strong radio bursts, a
Tenflare, a Type IV, and two separate occurrences of Type II radio
sweeps were also associated with this period of activity. LASCO
imagery depicted a full halo CME as a result of the complex series
of events that appears to have a fairly well connected Earth bound
component to the plasma cloud. This region has shown some growth
over the past 24 hours and has emerged into a beta-gamma-delta
magnetic complex. The largest flare of the period was an M4 that
occurred beyond the east limb at 18/1011Z and is thought to be from
old Region 486 which should start to become visible on day one of
the period. Region 507 (N10E78) was newly numbered today and is
believed to be old Region 488. Region 506 (S23E72) was also
numbered today.
IB. Voorspelling zonneactiviteit
Solar activity is expected to be at
moderate to high levels. Regions 501 and 507 are both capable of
producing major flare activity.
IIA. Samenvatting geofysische activiteit 17-2100Z tot 18-2100Z
The geomagnetic field was at unsettled to minor storm levels. The
elevated conditions are due to a favorably positioned recurrent high
speed coronal hole stream. The greater than 2 MeV electron fluxes
reached high levels today.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is
expected to range between predominantly active to minor storm levels
through much of the period. Minor storm conditions are expected
around the middle of day one due to a glancing blow, from the
partial halo CME that occurred as a result of the M4 flare that was
recorded at 0905Z on the 17 of Nov. Isolated major to severe storm
conditions are expected beginning around the middle of day two due
to a second transient that is expected as the result of the complex
M-class activity emanating a full halo CME today. Day three should
see a return to predominantly active conditions with isolated minor
storm possible at this time.
III. Kans zonnevlammen van 19 Nov tot 21 Nov
Klasse M | 70% | 80% | 80% |
Klasse X | 15% | 30% | 30% |
Proton | 10% | 15% | 20% |
PCAF | yellow
|
IV. Penticton 10.7 cm Flux
Geobserveerd 18 Nov 144
Voorspeld 19 Nov-21 Nov 160/190/220
90 dagen gemiddelde 18 Nov 129
V. Geomagnetische A index
Geobserveerd Afr/Ap 17 Nov 021/034
Geraamd Afr/Ap 18 Nov 018/021
Voorspeld Afr/Ap 19 Nov-21 Nov 025/040-040/050-030/030
VI. Kansen op geomagnetische activiteit van 19 Nov tot 21 Nov
A. Gemiddelde breedtegraad |
Actief | 40% | 40% | 55% |
Kleine storm | 20% | 35% | 25% |
Zware-ernstige stormcondities | 15% | 25% | 15% |
B. Hoge breedtegraad |
Actief | 30% | 20% | 40% |
Kleine storm | 40% | 50% | 35% |
Zware-ernstige stormcondities | 25% | 30% | 20% |
Alle tijden in UTC
<< Keer terug naar de dagelijkse overview pagina