Het archief bekijken van zondag 27 juni 1999
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 1999 Jun 27 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 178 gepubliceerd omstreeks 2200Z op 27 JUN 1999
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 26-2100Z tot 27-2100Z
SOLAR ACTIVITY WAS MODERATE. REGION 8592 (N22W33), A
SIMPLE SINGLE SPOT HSX GROUP, PRODUCED AN M1/2N FLARE TODAY AT
0844Z. THE EVENT WAS ACCOMPANIED BY A TYPE IV RADIO SWEEP. NEW
REGION 8611 (S26E60) EMERGED TODAY AND PRODUCED SOME SUBFLARE
ACTIVITY. REGION 8598 (N23W11) CONTINUES TO BE THE LARGEST REGION ON
THE DISK. THERE IS EVIDENCE OF EMERGING NEGATIVE MAGNETIC FLUX IN
THE MIDDLE OF A STRONG POSITIVE POLARITY FIELD WHICH HAS LED TO THE
FORMATION OF A DELTA SPOT NEAR THE CENTER OF THIS EXTENDED SUNSPOT
REGION. A VERY SLOW, LONG DURATION RISE AND DECAY IN THE X-RAY FLUX
OCCURRED BETWEEN 1815-2030Z, PEAKING AT THE C3 LEVEL; THE EVENT WAS
ASSOCIATED WITH SUBFAINT INTENSITY PLAGE IN REGION 8598. REGION 8602
(N17E22) AND 8603 (S16E29) ARE ALSO OF RESPECTABLE SIZE; BOTH
REGIONS PRODUCED A COUPLE SUBFLARES TODAY.
IB. Voorspelling zonneactiviteit
SOLAR ACTIVITY IS EXPECTED TO BE
MODERATE. REGION 8598 SHOWS GOOD POTENTIAL FOR PRODUCING M-CLASS
FLARES. REGIONS 8602, 8603, AND 8606 COULD ALSO POSSIBLY CONTRIBUTE
AN M-FLARE. THERE IS A POSSIBILITY FOR A MAJOR FLARE OR PROTON
PRODUCING FLARE FROM 8598.
IIA. Samenvatting geofysische activiteit 26-2100Z tot 27-2100Z
THE GEOMAGNETIC FIELD RANGED FROM QUIET TO ACTIVE LEVELS, WITH SOME
MINOR STORM INTERVALS AT HIGH LATITUDES. AN INITIALLY QUIET TO
UNSETTLED GEOMAGNETIC FIELD BECAME MORE DISTURBED AFTER 1200Z; AFTER
WHICH MIDDLE LATITUDES WERE MOSTLY ACTIVE AND HIGH LATITUDES WERE AT
ACTIVE TO MINOR STORM LEVELS. ACE OBSERVATIONS SHOW AN OSCILLATING
BZ COMPONENT WHICH BEGAN TO HAVE SOME NEGATIVE INTERVALS AFTER
0900Z.
IIB. Voorspelling geofysische activiteit
THE GEOMAGNETIC FIELD IS
EXPECTED TO PERSIST AT ACTIVE LEVELS FOR THE NEXT 12 HOURS, AFTER
WHICH UNSETTLED LEVELS ARE EXPECTED TO PREVAIL. UNSETTLED WITH A
POSSIBILITY FOR ACTIVE IS FORECAST FOR THE SECOND DAY BECAUSE A NEW
DISTURBANCE IS POSSIBLE ON THE 29TH DUE TO THE PARTIAL HALO CORONAL
MASS EJECTION THAT OCCURRED ON THE 24TH. GENERALLY UNSETTLED
CONDITIONS ARE EXPECTED TO PREDOMINATE ON THE THIRD DAY.
III. Kans zonnevlammen van 28 JUN tot 30 JUN
Klasse M | 75% | 75% | 75% |
Klasse X | 20% | 20% | 20% |
Proton | 25% | 25% | 25% |
PCAF | GREEN
|
IV. Penticton 10.7 cm Flux
Geobserveerd 27 JUN 207
Voorspeld 28 JUN-30 JUN 200/200/200
90 dagen gemiddelde 27 JUN 143
V. Geomagnetische A index
OBSERVED AFR/AP 26 JUN 014/017
ESTIMATED AFR/AP 27 JUN 018/020
PREDICTED AFR/AP 28 JUN-30 JUN 015/015-015/010-010/010
VI. Kansen op geomagnetische activiteit van 28 JUN tot 30 JUN
A. Gemiddelde breedtegraad |
Actief | 35% | 35% | 20% |
Kleine storm | 15% | 15% | 05% |
Zware-ernstige stormcondities | 05% | 05% | 01% |
B. Hoge breedtegraad |
Actief | 35% | 35% | 30% |
Kleine storm | 20% | 20% | 10% |
Zware-ernstige stormcondities | 10% | 10% | 05% |
Alle tijden in UTC
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