Het archief bekijken van dinsdag 9 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 09 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 314 gepubliceerd omstreeks 2200Z op 09 Nov 2004
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 08-2100Z tot 09-2100Z
Solar activity was high. Region 696 (N08W50) produced
several C-class flares and at 09/1719 UTC the region produced an
M8.9/2n Tenflare (1000 sfu), accompanied by Type II (1866 km/s) and
Type IV radio sweeps. A 23-degree fragmented filament erupted south
of the active region at the same time as the flare. The M8 flare
was also accompanied by a very fast asymmetric full halo CME on
LASCO imagery with a plane-of-sky speed of near 1800 km/s. Region
696 maintained a beta-gamma-delta magnetic configuration. Region
698 (S09W84) produced several C-class flares during the period.
Region 699 (S16E66) was numbered today. The 10 cm flux value
observed today was flare enhanced.
IB. Voorspelling zonneactiviteit
Solar activity is expected to be
moderate to high. Region 696 is expected to produce M-class flares,
and X-class flares are possible.
IIA. Samenvatting geofysische activiteit 08-2100Z tot 09-2100Z
The geomagnetic field has been at unsettled to severe storm
conditions. The period began with active to major storm levels with
solar wind speed elevated to 600 km/s. A 34 nT sudden impulse was
observed at 09/0931 UTC, which was followed by major to severe
storming and an increase of solar wind speed from 600 to 800 km/s.
Another sudden impulse (46 nT) was observed at 1852 UTC and was
followed by severe storm conditions to the end of the period. The
GOES 10 and 12 spacecraft observed magnetopause crossings following
the second sudden impulse. Solar wind speed increased from 650 to
800 km/s and Bz turned southward to 30 nT for over an hour. The
greater than 10 MeV proton event that began on 07/1910 UTC continued
into the period, and the proton flux ended the period at 55 pfu.
The greater than 2 MeV electron flux at GOES was at high levels
today.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is
expected to be at unsettled to major storm conditions on 10-11
November. A CME shock associated with the M8 flare observed today
should arrive on 11 November. Activity should subside to quiet to
active levels on 12 November.
III. Kans zonnevlammen van 10 Nov tot 12 Nov
Klasse M | 75% | 70% | 65% |
Klasse X | 20% | 20% | 15% |
Proton | 99% | 25% | 15% |
PCAF | in progress
|
IV. Penticton 10.7 cm Flux
Geobserveerd 09 Nov 141
Voorspeld 10 Nov-12 Nov 120/115/110
90 dagen gemiddelde 09 Nov 110
V. Geomagnetische A index
Geobserveerd Afr/Ap 08 Nov 116/189
Geraamd Afr/Ap 09 Nov 085/100
Voorspeld Afr/Ap 10 Nov-12 Nov 030/040-045/050-015/015
VI. Kansen op geomagnetische activiteit van 10 Nov tot 12 Nov
A. Gemiddelde breedtegraad |
Actief | 35% | 40% | 30% |
Kleine storm | 25% | 35% | 20% |
Zware-ernstige stormcondities | 20% | 25% | 10% |
B. Hoge breedtegraad |
Actief | 45% | 30% | 45% |
Kleine storm | 30% | 40% | 25% |
Zware-ernstige stormcondities | 20% | 30% | 10% |
Alle tijden in UTC
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