Het archief bekijken van zaterdag 2 mei 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 May 02 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 122 gepubliceerd omstreeks 2200Z op 02 MAY 1998
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 01-2100Z tot 02-2100Z
SOLAR ACTIVITY HAS BEEN HIGH FOR THE PAST 24 HOURS.
REGION 8210 (S17W21) PRODUCED AN X1/3B TENFLARE (1300 FLUX UNITS)
THAT REACHED MAXIMUM AT 02/1342 UT. IT WAS ACCOMPANIED BY A
PARTIAL-HALO CORONAL MASS EJECTION (REPORTED BY SOHO/LASCO
OPERATIONS), SIGNIFICANT RADIO BURSTS ACROSS THE SPECTRUM AND A TYPE
IV SWEEP. THE CME WAS CONCENTRATED OFF THE NW LIMB AND THE MEASURED
SPEED WAS APPROXIMATELY 750 KM/S. REGION 8210 ALSO PARTICIPATED IN
AN M1 X-RAY EVENT ON 01/2254 UT SHARED WITH REGION 8214 (N27E19).
THIS EARLIER EVENT MAY ALSO BE ASSOCIATED WITH A PARTIAL-HALO CME
CONCENTRATED OFF THE NE LIMB. REGION 8210 IS EXTREMELY MAGNETICALLY
COMPLEX, AND REGIONS 8210 AND 8214 ARE BOTH CONTINUING TO GROW IN
SIZE AND SPOT COUNT. NEW REGION 8217 (S17E77), A SIMPLE A-TYPE
GROUP, WAS NUMBERED TODAY. THERE ARE CONTINUING INDICATIONS OF
ACTIVE REGIONS BEYOND THE EAST LIMB THAT WILL BE ROTATING ONTO THE
DISK IN THE NEXT FEW DAYS.
IB. Voorspelling zonneactiviteit
SOLAR ACTIVITY IS EXPECTED TO PERSIST
AT MODERATE TO HIGH LEVELS. REGION 8210 RETAINS THE EXTREME MAGNETIC
COMPLEXITY ASSOCIATED WITH MAJOR X-RAY EVENTS, AND THE PROBABILITY
OF SIGNIFICANT ACTIVITY FROM REGION 8214 IS INCREASING AS IT
CONTINUES TO DEVELOP.
IIA. Samenvatting geofysische activiteit 01-2100Z tot 02-2100Z
GEOMAGNETIC ACTIVITY REACHED PERIODS AT MAJOR STORM LEVELS DURING THE
PAST 24 HOURS. THE STORM SUDDEN COMMENCEMENT OCCURRED AT 01/2158 UT.
IT IS PRESUMED TO HAVE ORIGINATED WITH A MAJOR SOLAR EVENT ON 29
APRIL. PRECEDING THE SSC, THE PASSAGE OF AN INTERPLANETARY SHOCK WAS
OBSERVED IN ACE SOLAR WIND DATA AT APPROXIMATELY 01/2124 UT. A
GREATER THAN 100 MEV SATELLITE PROTON EVENT BEGAN 02/1405 AND
REACHED 7.6 PFU AT 1540 UT. A GREATER THAN 10 MEV SATELLITE PROTON
EVENT BEGAN AT 02/1420UT AND REACHED 150 PFU AT 1650 UT. BOTH
EVENTS ARE STILL IN PROGRESS AT REPORT ISSUE TIME. A POLAR CAP
ABSORPTION EVENT IS IN PROGRESS, AS WELL AS A FORBUSH DECREASE OF
APPROXIMATELY 5 PERCENT.
IIB. Voorspelling geofysische activiteit
GEOMAGNETIC ACTIVITY IS
EXPECTED TO DECLINE TOWARD GENERALLY UNSETTLED TO ACTIVE CONDITIONS
TOMORROW, BUT A NEW STORM COMMENCEMENT IS EXPECTED AFTER MIDDAY ON
04 MAY FROM THE X-CLASS SOLAR ACTIVITY ON 02 MAY. MAJOR STORM
CONDITIONS ARE PROBABLE ON 05 MAY. THE SATELLITE PROTON EVENT AT
GREATER THAN 10 MEV ENERGIES IS EXPECTED TO PERSIST THROUGH 04 MAY,
AND COULD CONTINUE LONGER IF NEW SOLAR ACTIVITY OCCURS.
III. Kans zonnevlammen van 03 MAY tot 05 MAY
Klasse M | 50% | 50% | 50% |
Klasse X | 30% | 30% | 30% |
Proton | 30% | 30% | 30% |
PCAF | IN PROGRESS
|
IV. Penticton 10.7 cm Flux
Geobserveerd 02 MAY 117
Voorspeld 03 MAY-05 MAY 130/140/150
90 dagen gemiddelde 02 MAY 104
V. Geomagnetische A index
OBSERVED AFR/AP 01 MAY 008/008
ESTIMATED AFR/AP 02 MAY 045/060
PREDICTED AFR/AP 03 MAY-05 MAY 020/035-020/020-050/050
VI. Kansen op geomagnetische activiteit van 03 MAY tot 05 MAY
A. Gemiddelde breedtegraad |
Actief | 30% | 25% | 10% |
Kleine storm | 25% | 15% | 20% |
Zware-ernstige stormcondities | 11% | 21% | 60% |
B. Hoge breedtegraad |
Actief | 25% | 35% | 10% |
Kleine storm | 30% | 20% | 20% |
Zware-ernstige stormcondities | 16% | 11% | 60% |
Alle tijden in UTC
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