Het archief bekijken van woensdag 19 juli 2000
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 2000 Jul 19 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 201 gepubliceerd omstreeks 2200Z op 19 JUL 2000
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 18-2100Z tot 19-2100Z
SOLAR ACTIVITY BECAME HIGH. REGION 9087 (S12W00)
PRODUCED A LONG DURATION M6/3N FLARE AT 19/0726Z. MINOR RADIO
BURSTS, INCLUDING A WEAK TYPE IV, ACCOMPANIED THIS EVENT. NO
CORONAGRAPH DATA WERE AVAILABLE FROM SOHO BUT IT IS ASSUMED THAT
THERE WAS A SIGNIFICANT MASS EJECTION WITH THIS EVENT BECAUSE OF
SOFT X-RAY DURATION AND INTERPLANETARY PARTICLE FLUXES. REGION 9087
CONTINUED TO EMERGE RAPIDLY IN ITS NEW LEADER AREA AND TO THE SOUTH
OF THE PREEXISTING SPOTS. THE DELTA CONFIGURATION REMAINED. REGION
9097 (N05E67) SHOWED ITSELF AS A MODERATELY LARGE CLASS D SUNSPOT
REGION AND PRODUCED OCCASIONAL SUBFLARES. REGION 9077 (N19W72)
CONTINUED TO DECLINE AND PRODUCED ONLY INFREQUENT SUBFLARES.
IB. Voorspelling zonneactiviteit
SOLAR ACTIVITY IS EXPECTED TO BECOME
GENERALLY HIGH. THE CONTINUED GROWTH IN AREA AND MAGNETIC
COMPLEXITY IN REGION 9087 MAKES IT THE PRIME CANDIDATE FOR A MAJOR
EVENT. LESSER FLARES MAY COME FROM REGIONS 9077 AND 9097.
IIA. GEOPHYSICAL ACTIVITY SUMMARY 18/2100Z TO 19/2100Z:
THE GEOMAGNETIC FIELD WAS QUIET TO UNSETTLED FOR MOST OF THE PERIOD.
A SHOCK WAS OBSERVED AT ACE AT 19/1450Z AND A SUDDEN IMPULSE WAS
OBSERVED AT THE EARTH AT 19/1526Z. UNSETTLED TO ACTIVE CONDITIONS
FOLLOWED THE SHOCK PASSAGE. SOLAR WIND VELOCITY JUMPED FROM
APPROXIMATELY 450 KM/S TO OVER 600 KM/S. THE LIKELY SOURCE OF THIS
DISTURBANCE WAS A MASS EJECTION ON 17 JULY THAT APPEARED TO BE
DIRECTED OFF THE EAST LIMB OF THE SUN. THE GREATER THAN 10 MEV FLUX
BEGAN THE PERIOD NEAR 20 PFU AND DECAYED TO NEAR 10 PFU AT THE END
OF THE PERIOD. A SLIGHT INCREASE IN FLUX WAS OBSERVED AROUND
19/1500Z WHICH MAY HAVE BEEN RELATED TO THE M6 FLARE MENTIONED
ABOVE.
IIB. Voorspelling geofysische activiteit
THE GEOMAGNETIC FIELD SHOULD
RANGE BETWEEN QUIET AND ACTIVE LEVELS FOR 20 JULY. ACTIVE TO MAJOR
STORM LEVELS ARE EXPECTED ON 21 JULY IN RESPONSE TO TODAY'S
SUSPECTED MASS EJECTION. UNSETTLED TO ACTIVE LEVELS SHOULD RETURN ON
22 JULY. THE CURRENT SOLAR PROTON EVENT COULD END ON 20 JULY.
HOWEVER, THE LARGE FLARES EXPECTED FROM REGION 9087 WILL LIKELY
CAUSE NEW INJECTIONS OF ENERGETIC PROTONS DURING THE PERIOD.
III. Kans zonnevlammen van 20 JUL tot 22 JUL
Klasse M | 90% | 90% | 90% |
Klasse X | 50% | 50% | 50% |
Proton | 50% | 50% | 50% |
PCAF | YELLOW
|
IV. Penticton 10.7 cm Flux
Geobserveerd 19 JUL 250
Voorspeld 20 JUL-22 JUL 252/245/235
90 dagen gemiddelde 19 JUL 188
V. Geomagnetische A index
OBSERVED AFR/AP 18 JUL 008/013
ESTIMATED AFR/AP 19 JUL 012/014
PREDICTED AFR/AP 20 JUL-22 JUL 020/015-050/040-020/015
VI. Kansen op geomagnetische activiteit van 20 JUL tot 22 JUL
A. Gemiddelde breedtegraad |
Actief | 40% | 25% | 40% |
Kleine storm | 15% | 25% | 15% |
Zware-ernstige stormcondities | 10% | 30% | 10% |
B. Hoge breedtegraad |
Actief | 40% | 25% | 40% |
Kleine storm | 15% | 25% | 15% |
Zware-ernstige stormcondities | 10% | 30% | 10% |
Alle tijden in UTC
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