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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 Aug 16 2200 UTC
Preparati dal SWPC della NOAA© ed elaborati da SpaceWeatherLive.comRapporto Congiunto USAF/NOAA dell'Attività Solare e Geofisica
SDF Numero 228 Emesso alle 2200Z il Aug 16 2001
IA. Analisi delle Regioni Solari Attive e Attività dalle 2100Z-15 alle 2100Z-16
Solar activity from numbered regions on the visible
disk was low. Impulsive B- and C-class flares were observed
throughout the period, the largest being an optically uncorrelated
C3 flare at 16/0957 UTC. However, the most impressive activity of
the day was a remarkable backside CME, observed on SOHO/LASCO
starting at about 15/2355 UTC. This event resulted in the proton
enhancements discussed in section IIA below. The observed CME
together with backside imagery inferred from the SOHO/MDI instrument
suggest old Region 9557 (S20, L=283) as the likely source, presently
located near the far backside central meridian. On the visible
disk, three new regions were numbered today: 9583 (S23E13), 9584
(S11E60), and 9585 (N15E74). All appear to be small, simply
structured beta-class groups with low flare activity potential.
IB. Previsione dell'Attività Solare
Solar activity on the visible disk is
expected to persist at mainly low levels for the next three days.
IIA. Sommario dell'Attività Geofisica dalle 2100Z-15 alle 2100Z-16
Geomagnetic field activity has been quiet to unsettled throughout the
period. A major proton event for >= 100MeV protons above 1pfu began
at 16/0105 UTC, followed by >= 10Mev protons above 10pfu at 16/0135
UTC. Maximum flux for 100Mev protons was 29pfu at 16/0305 UTC, and
for 10MeV protons was 493pfu at 16/0355 UTC. Both events remain in
progress, and represent a record response for a presumed CME source
so far behind the western limb as described in section 1A above.
Greater than 2MeV electrons were observed at moderate enhancement
levels again today, although the electron sensor on GOES-8 was
saturated by the proton event for much of the period.
IIB. Previsione dell'Attività Geofisica
The geomagnetic field is
expected to be at active to minor storm levels within 24 hours, in
response to anticipated shock passage from CME activity reported on
August 14th. Isolated major storm periods may also be possible at
higher latitudes, as well as an enhancement of 10MeV proton levels
for the event in progress. Geomagnetic storm activity is expected
to wane during day two, along with the 100MeV proton event. The
10MeV proton event is expected to persist at levels above 10pfu into
day three. Greater than 2MeV electrons are also expected to persist
at moderate enhancement levels.
III. Probabilità dell'Evento dalle Aug del 17 alle Aug del 19
Classe M | 25% | 25% | 25% |
Classe X | 01% | 01% | 01% |
Protone | 99% | 95% | 90% |
PCAF | red
|
IV. Flusso di 10.7 cm di Penticton
Osservato 16 Aug 143
Previsto 17 Aug-19 Aug 140/140/145
Media di 90 Giorni 16 Aug 151
V. Indici Geomagnetici A
Osservato Afr/Ap 15 Aug 004/009
Stimato Afr/Ap 16 Aug 007/008
Previsto Afr/Ap 17 Aug-19 Aug 025/020-017/015-012/018
VI. Probabilità dell'Attività Geomagnetica dal 17 Aug al 19 Aug
A. Latitudini Medie |
Attivo | 35% | 30% | 25% |
Tempesta minore | 20% | 15% | 10% |
Tempesta maggiore-grave | 10% | 05% | 05% |
B. Latitudini Alte |
Attivo | 40% | 30% | 30% |
Tempesta minore | 20% | 15% | 15% |
Tempesta maggiore-grave | 05% | 05% | 05% |
Tutti gli orari in UTC
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