Het archief bekijken van donderdag 10 mei 2012
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 2012 May 10 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 131 gepubliceerd omstreeks 2200Z op 10 May 2012
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 09-2100Z tot 10-2100Z
Solar activity has been at high levels for the past 24
hours with multiple M-class solar flares observed. Region 1476
(N12E08) was responsible for almost all of the activity with 3
M-class events observed, the largest being a M5/2b event at
10/0418Z. Associated with these events, were discrete frequency
radio bursts, Tenflares, and even a Type IV radio sweep. Region 1476
has shown mixed growth and shear effects across the polarities as it
continues to evolve. A weak Earth directed CME was observed in
STEREO COR2 A and B imagery early in the period. Analysis and
current models show this CME joining the current coronal hole high
speed stream (CH HSS). Region 1477 (S22E47) was split into two
regions today as SDO magnetogram data indicated the leader and
follower sunspot groups were actually two magnetic bipoles. Leader
group is Region 1477 and follower group is now Region 1478 (S24E55).
IB. Voorspelling zonneactiviteit
Solar activity is expected to be at
moderate levels with a slight chance for X-class events for the next
three days (11 - 13 May) as Region 1476 continues to grow and
evolve.
IIA. Samenvatting geofysische activiteit 09-2100Z tot 10-2100Z
The geomagnetic field has been at quiet to active levels for the past
24 hours with an isolated minor storm period observed at high
latitudes. Solar wind measurements, as observed by the ACE
spacecraft, showed a continued increase in solar wind speeds to
around 620 km/s, a drop off in solar wind density, and the total IMF
began to stabilize around 5 nT. These characteristics are indicative
of a CH HSS. The greater than 2 MeV electron flux at geosynchronous
orbit reached high levels during the period.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is
expected to be at quiet to unsettled levels with a chance for active
periods for the next three days (11 - 13 May). The increased
activity is due to both the continued CH HSS effects and three weak,
slow moving CMEs intertwined within.
III. Kans zonnevlammen van 11 May tot 13 May
Klasse M | 75% | 75% | 75% |
Klasse X | 20% | 20% | 20% |
Proton | 10% | 10% | 10% |
PCAF | Green
|
IV. Penticton 10.7 cm Flux
Geobserveerd 10 May 131
Voorspeld 11 May-13 May 130/130/130
90 dagen gemiddelde 10 May 113
V. Geomagnetische A index
Geobserveerd Afr/Ap 09 May 019/025
Geraamd Afr/Ap 10 May 010/010
Voorspeld Afr/Ap 11 May-13 May 012/012-010/012-006/010
VI. Kansen op geomagnetische activiteit van 11 May tot 13 May
A. Gemiddelde breedtegraad |
Actief | 20% | 20% | 15% |
Kleine storm | 05% | 05% | 01% |
Zware-ernstige stormcondities | 01% | 01% | 01% |
B. Hoge breedtegraad |
Actief | 40% | 40% | 30% |
Kleine storm | 10% | 10% | 10% |
Zware-ernstige stormcondities | 01% | 01% | 01% |
Alle tijden in UTC
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