Het archief bekijken van dinsdag 28 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 28 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 118 gepubliceerd omstreeks 2200Z op 28 APR 1998
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 27-2100Z tot 28-2100Z
SOLAR ACTIVITY DROPPED PRECIPITOUSLY TO A VERY LOW
LEVEL. ONLY B-CLASS ENHANCEMENTS WERE OBSERVED. REGION 8210 (S17E31)
RETAINED ITS DELTA CONFIGURATION, DEVELOPED ADDITIONAL MIXED
POLARITIES, AND EXHIBITED MINOR GROWTH. H-ALPHA FIBRIL AND VECTOR
MAGNETOGRAPH DATA INDICATE STRONG SHEAR IN THIS REGION WHERE THE
DELTA IS LOCATED. A FILAMENT IN THIS REGION FADED RAPIDLY BETWEEN
28/1851-1914Z. TWO SMALL REGIONS EMERGED ON THE DISK NEAR S30W64 AND
S25E55 AND WERE NUMBERED AS REGIONS 8212 AND 8213 RESPECTIVELY.
IB. Voorspelling zonneactiviteit
SOLAR ACTIVITY SHOULD BECOME LOW TO
MODERATE DURING THE NEXT THREE DAYS. REGION 8210 RETAINS THE
CAPABILITY OF PRODUCING ANOTHER SMALL X-CLASS EVENT. OLD REGION 8194
WILL BE RETURNING TO THE EAST LIMB NEAR S18 AROUND 01 MAY. THIS
REGION PRODUCED A LONG DURATION M1 FLARE ON 20 APR FROM SEVERAL DAYS
BEYOND THE WEST LIMB THAT RESULTED IN A LARGE SOLAR PROTON EVENT AT
EARTH. ACTIVITY LEVELS MAY INCREASE UPON THE RETURN OF THIS REGION.
IIA. Samenvatting geofysische activiteit 27-2100Z tot 28-2100Z
THE GEOMAGNETIC FIELD WAS QUIET TO UNSETTLED. SOLAR WIND VELOCITIES
DECREASED DURING THE PERIOD TO BELOW 400 KM/S INDICATING AN END OF
THE CORONAL HOLE RELATED DISTURBANCE OF THE LAST SEVERAL DAYS.
ENERGETIC ELECTRON FLUXES AT GEOSYNCHRONOUS ORBIT WERE PREDOMINANTLY
HIGH.
IIB. Voorspelling geofysische activiteit
THE GEOMAGNETIC FIELD SHOULD BE
QUIET TO UNSETTLED UNTIL NEAR MIDDAY ON 29 APR WHEN A HALO CME
RELATED DISTURBANCE IS EXPECTED TO BEGIN. UNSETTLED TO MINOR STORM
CONDITIONS SHOULD BE EXPERIENCED FROM THAT TIME AND THROUGH 30 APR.
ISOLATED PERIODS OF MAJOR STORMING ARE POSSIBLE. PREDOMINANTLY
UNSETTLED TO ACTIVE CONDITIONS ARE EXPECTED ON 01 MAY AS THE
DISTURBANCE PASSES THE EARTH.
III. Kans zonnevlammen van 29 APR tot 01 MAY
| Klasse M | 20% | 20% | 25% |
| Klasse X | 15% | 15% | 15% |
| Proton | 15% | 15% | 15% |
| PCAF | GREEN
|
IV. Penticton 10.7 cm Flux
Geobserveerd 28 APR 098
Voorspeld 29 APR-01 MAY 099/100/103
90 dagen gemiddelde 28 APR 104
V. Geomagnetische A index
OBSERVED AFR/AP 27 APR 012/014
ESTIMATED AFR/AP 28 APR 010/015
PREDICTED AFR/AP 29 APR-01 MAY 020/020-020/020-015/015
VI. Kansen op geomagnetische activiteit van 29 APR tot 01 MAY
| A. Gemiddelde breedtegraad |
| Actief | 30% | 30% | 25% |
| Kleine storm | 30% | 30% | 15% |
| Zware-ernstige stormcondities | 10% | 10% | 05% |
| B. Hoge breedtegraad |
| Actief | 30% | 30% | 25% |
| Kleine storm | 35% | 40% | 15% |
| Zware-ernstige stormcondities | 15% | 15% | 05% |
Alle tijden in UTC
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