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Rapporto attività solare
Ogni brillamento solare menzionato nel rapporto ha un fattore di scala, applicato dal Centro di Predizione Meteorologica Spaziale (SWPC). A causa del fattore di scala del SWPC, i brillamenti solari sono segnalati come ridotti del 42%, rispetto ai dati di qualità scientifica. Il fattore di scala è stato rimosso dai nostri dati archiviati sui brillamenti solari, per riflettere le unità fisiche reali.
Rapporto dell'Attività Geofisica Solare 1998 May 05 2200 UTC
Preparati dal SWPC della NOAA© ed elaborati da SpaceWeatherLive.comRapporto Congiunto USAF/NOAA dell'Attività Solare e Geofisica
SDF Numero 125 Emesso alle 2200Z il MAY 05 1998
IA. Analisi delle Regioni Solari Attive e Attività dalle 2100Z-04 alle 2100Z-05
SOLAR ACTIVITY HAS BEEN LOW. THE DAY'S EVENTS CONSISTED
OF OCCASIONAL C-CLASS FLARES. THE LARGEST OF THESE WAS A C7.3 AT
1938Z. THE SOURCE FOR MOST OF THE ACTIVITY WAS REGION 8214 (N27W31).
THIS REGION IS GROWING AND HAS BRIGHT PLAGE WITH FREQUENT
FLUCTUATIONS. OBSERVERS ARE REPORTING GROWTH AND DEVELOPMENT OF
PENUMBRA IN THE INTERMEDIATE SPOTS. THE CURRENT MAGNETIC
CONFIGURATION IS MORE COMPLEX TODAY (BETA-GAMMA) AND THE REGION IS
BECOMING COMPACT. REGION 8210 (S17W60) WAS RELATIVELY CALM TODAY,
SHOWED A SLIGHT INCREASE IN AREA, BUT WAS REPORTED TO PRODUCE ONLY A
FEW SUBFLARES.
IB. Previsione dell'Attività Solare
SOLAR ACTIVITY IS EXPECTED TO BE
MODERATE. THERE IS A GOOD CHANCE FOR AN M-CLASS EVENT FROM REGION
8214. THERE IS ALSO A POSSIBILITY FOR A MAJOR FLARE FROM THIS
REGION, ESPECIALLY IF THE CURRENT TRENDS CONTINUE. REGION 8210
CONTINUES TO POSE A FAIR M-CLASS THREAT AS WELL.
IIA. Sommario dell'Attività Geofisica dalle 2100Z-04 alle 2100Z-05
THE GEOMAGNETIC FIELD HAS RANGED FROM UNSETTLED TO MAJOR STORM LEVELS
OVER THE PAST 24 HOURS. AN INITIALLY UNSETTLED TO ACTIVE FIELD
BECAME DISTURBED BETWEEN 0300-0700Z, WITH MAJOR STORM CONDITIONS
OBSERVED AT MID AND HIGH LATITUDE STATIONS. FROM 0700-2100Z THE
FIELD HAS BEEN CHARACTERIZED BY PREDOMINANTLY ACTIVE LEVELS, WITH
SOME MINOR STORM PERIODS AT THE HIGH LATITUDE STATIONS. THE MAJOR
GEOMAGNETIC STORM THAT BEGAN WITH THE SSC OF 04/0300Z OFFICIALLY
ENDED AT 05/0900UT. THE CURRENT ACTIVITY IS ASSOCIATED WITH THE
X1/3B/HALO CME EVENT OF 02/1342Z. THIS EVENT WAS INITIALLY SEEN AT
ACE AS A STRONG SHOCK AT 04/0229Z FOLLOWED BY A PERIOD OF NEGATIVE
BZ FROM 04/0230-0430Z. THE SOLAR WIND DATA HAVE CONTINUED TO SHOW
CHARACTERISTICS OF TRANSIENT FLOW OVER THE PAST 24 HOURS, NAMELY
STRONG MAGNETIC FIELDS, VARIABLE TEMPERATURES, AND VARIABLE BUT HIGH
VELOCITIES. THE FLOW DOES NOT SHOW THE 'CLASSIC CLOUD' STRUCTURE,
SUGGESTING THAT THE DRIVER MISSED HITTING THE EARTH DIRECTLY. THE
GREATER THAN 2 MEV ELECTRONS EXCEEDED HIGH LEVELS DURING THE PAST 24
HOURS.
IIB. Previsione dell'Attività Geofisica
THE GEOMAGNETIC FIELD IS
EXPECTED TO BE PREDOMINANTLY ACTIVE FOR THE NEXT 24-36 HOURS DUE TO
LINGERING EFFECTS OF THE CURRENT DISTURBANCE. CONDITIONS SHOULD
RETURN TO UNSETTLED TO QUIET THEREAFTER.
III. Probabilità dell'Evento dalle MAY del 06 alle MAY del 08
Classe M | 75% | 75% | 75% |
Classe X | 20% | 20% | 20% |
Protone | 20% | 20% | 20% |
PCAF | YELLOW
|
IV. Flusso di 10.7 cm di Penticton
Osservato 05 MAY 133
Previsto 06 MAY-08 MAY 135/135/130
Media di 90 Giorni 05 MAY 106
V. Indici Geomagnetici A
OBSERVED AFR/AP 04 MAY 090/096
ESTIMATED AFR/AP 05 MAY 025/035
PREDICTED AFR/AP 06 MAY-08 MAY 020/025-015/020-005/013
VI. Probabilità dell'Attività Geomagnetica dal 06 MAY al 08 MAY
A. Latitudini Medie |
Attivo | 20% | 20% | 10% |
Tempesta minore | 10% | 05% | 05% |
Tempesta maggiore-grave | 10% | 05% | 05% |
B. Latitudini Alte |
Attivo | 25% | 25% | 10% |
Tempesta minore | 10% | 05% | 05% |
Tempesta maggiore-grave | 10% | 05% | 05% |
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