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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 2001 Nov 04 2200 UTC
Preparati dal SWPC della NOAA© ed elaborati da SpaceWeatherLive.comRapporto Congiunto USAF/NOAA dell'Attività Solare e Geofisica
SDF Numero 308 Emesso alle 2200Z il Nov 04 2001
IA. Analisi delle Regioni Solari Attive e Attività dalle 2100Z-03 alle 2100Z-04
Solar activity has been high. Region 9684 (N06W27)
produced an X1/3b flare beginning at 1603 UTC, maximum at 1620 UTC,
and ending at 1647 UTC. The event was accompanied by strong radio
bursts, a type II sweep, and a type IV sweep. A CME was observed to
enter the C2 field of view during the flare, with the leading edge
just visible at 1635 UTC. The front edge moved quickly across C2 and
exited somewhere between 1655 UTC and 1705 UTC. Region 9684 has
grown and the leader and trailer spots merged during the past 24
hours, making the region a beta-gamma-delta group. Region 9687
(S20E35) continues to be a complex, beta-gamma group and produced a
few C-class subflares. Region 9682 (N13W64) is still the largest
group on the disk but could only muster a couple of subflares. A 10
degree filament just west of Region 9684 disappeared sometime
between 03/2208 UTC and 04/0629 UTC.
IB. Previsione dell'Attività Solare
Solar activity is expected to be
moderate to high. M-class events are likely to occur during the next
three days. There is a fair chance for an additional major flare
from Region 9684, especially if new magnetic flux continues to
emerge. Regions 9682 and 9687 also continue to pose a slight threat
for major flare activity.
IIA. Sommario dell'Attività Geofisica dalle 2100Z-03 alle 2100Z-04
The geomagnetic field was quiet to unsettled during the past 24
hours. A greater than 100 MeV proton event began at 1650 UTC,
shortly after today's X-class flare. Flux levels rose quickly
initially, but began to level off around 1800 UTC, although they are
still climbing slowly. The maximum 100 MeV flux observed so far is
56 pfu at 2035 UTC. A greater than 10 MeV proton event began at 1705
UTC. This event also seems to be leveling off, and the maximum flux
observed so far is 1180 pfu at 2040 UTC.
IIB. Previsione dell'Attività Geofisica
The geomagnetic field is
expected to be unsettled to slightly active tomorrow. Major storm
conditions are likely to follow the arrival of a shock from today's
solar event, sometime early on the 2nd day (06 November). The
disturbance is expected to last for about 24 hours, and a decrease
to mostly active conditions should occur on the third day. Today's
greater than 100 MeV proton event is expected to continue for the
next 12 hours. The greater than 10 MeV proton event should continue
tomorrow, and is likely to get an enhancement of flux levels on the
second day with the arrival of the interplanetary shock from today's
solar event.
III. Probabilità dell'Evento dalle Nov del 05 alle Nov del 07
Classe M | 80% | 80% | 80% |
Classe X | 25% | 25% | 25% |
Protone | 99% | 80% | 25% |
PCAF | in progress
|
IV. Flusso di 10.7 cm di Penticton
Osservato 04 Nov 227
Previsto 05 Nov-07 Nov 220/215/210
Media di 90 Giorni 04 Nov 206
V. Indici Geomagnetici A
Osservato Afr/Ap 03 Nov 001/003
Stimato Afr/Ap 04 Nov 007/008
Previsto Afr/Ap 05 Nov-07 Nov 015/015-050/050-025/025
VI. Probabilità dell'Attività Geomagnetica dal 05 Nov al 07 Nov
A. Latitudini Medie |
Attivo | 25% | 10% | 20% |
Tempesta minore | 15% | 15% | 35% |
Tempesta maggiore-grave | 15% | 75% | 35% |
B. Latitudini Alte |
Attivo | 25% | 05% | 15% |
Tempesta minore | 15% | 10% | 30% |
Tempesta maggiore-grave | 15% | 80% | 35% |
Tutti gli orari in UTC
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