Het archief bekijken van maandag 27 april 1998
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 1998 Apr 27 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 117 gepubliceerd omstreeks 2200Z op 27 APR 1998
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 26-2100Z tot 27-2100Z
SOLAR ACTIVITY BECAME HIGH. REGION 8210 (S17E43)
PRODUCED AN X1/2B AT 27/0920Z WITH A STRONG TYPE IV AND 950 SFU
BURST AT 2695 MHZ. THIS MODERATE DURATION EVENT WAS ACCOMPANIED BY A
CORONAL MORETON WAVE AND HALO CORONAL MASS EJECTION. REGION 8210
REMAINED A SMALL-MODERATE SIZE C-CLASS GROUP. HOWEVER, A MAGNETIC
DELTA CONFIGURATION FORMED IN THE NORTHERN PORTION OF THE REGION AND
LOCALIZED MAGNETIC GRADIENTS WERE HIGH. SMALL REGIONS WERE VISIBLE
NEARING THE NORTHEAST AND SOUTHEAST LIMBS.
IB. Voorspelling zonneactiviteit
SOLAR ACTIVITY SHOULD BE LOW TO
OCCASIONALLY MODERATE WITH REGION 8210 THE PROBABLE SOURCE REGION.
OBVIOUSLY, X-CLASS EVENTS ARE POSSIBLE BUT NOT CONSIDERED LIKELY DUE
TO THE SMALL AREAL COVERAGE OF THIS REGION IN WHITE LIGHT. CONTINUED
INCREASES IN MAGNETIC COMPLEXITY COULD MODIFY THIS FORECAST.
IIA. Samenvatting geofysische activiteit 26-2100Z tot 27-2100Z
THE GEOMAGNETIC FIELD RANGED FROM UNSETTLED TO MINOR STORM LEVELS.
THE MOST DISTURBED PERIOD WAS FROM 27/0000-0300Z. THIS DISTURBANCE
APPEARS TO BE CAUSED BY AN EXTENSION OF THE SOUTHERN POLAR CORONAL
HOLE. ENERGETIC ELECTRON FLUXES AT GEOSYNCHRONOUS ORBIT WERE
PREDOMINANTLY HIGH.
IIB. Voorspelling geofysische activiteit
THE GEOMAGNETIC FIELD SHOULD BE
UNSETTLED TO SLIGHTLY ACTIVE ON 28 APR AS THE END OF THE CORONAL
HOLE STREAM ROTATES PAST THE EARTH DURING THAT PERIOD. UNSETTLED TO
MINOR STORM CONDITIONS ARE PREDICTED FOR 29-30 APR IN RESPONSE TO
THE X1 FLARE AND HALO CME MENTIONED ABOVE. ISOLATED PERIODS OF MAJOR
STORMING ARE POSSIBLE AT HIGH LATITUDES. THE ARRIVAL TIME FOR THIS
DISTURBANCE IS SOMEWHAT ADVANCED FROM PREVIOUS HALO CMES DUE TO A
HIGH LAUNCH SPEED OBSERVED NEAR THE SUN.
III. Kans zonnevlammen van 28 APR tot 30 APR
Klasse M | 20% | 20% | 20% |
Klasse X | 15% | 15% | 15% |
Proton | 10% | 15% | 15% |
PCAF | GREEN
|
IV. Penticton 10.7 cm Flux
Geobserveerd 27 APR 091
Voorspeld 28 APR-30 APR 092/094/096
90 dagen gemiddelde 27 APR 104
V. Geomagnetische A index
OBSERVED AFR/AP 26 APR 021/031
ESTIMATED AFR/AP 27 APR 015/020
PREDICTED AFR/AP 28 APR-30 APR 010/015-020/020-020/020
VI. Kansen op geomagnetische activiteit van 28 APR tot 30 APR
A. Gemiddelde breedtegraad |
Actief | 20% | 30% | 35% |
Kleine storm | 10% | 20% | 25% |
Zware-ernstige stormcondities | 05% | 10% | 10% |
B. Hoge breedtegraad |
Actief | 25% | 35% | 35% |
Kleine storm | 15% | 25% | 30% |
Zware-ernstige stormcondities | 05% | 15% | 15% |
Alle tijden in UTC
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