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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 2012 Jul 17 2200 UTC
Preparati dal SWPC della NOAA© ed elaborati da SpaceWeatherLive.comRapporto Congiunto USAF/NOAA dell'Attività Solare e Geofisica
SDF Numero 199 Emesso alle 2200Z il Jul 17 2012
IA. Analisi delle Regioni Solari Attive e Attività dalle 2100Z-16 alle 2100Z-17
Solar activity was moderate. Todays activity was
dominated by a very long-duration M1 flare that occurred between
1203-1904Z with maximum at 1715Z. The source region appeared to
primarily be Region 1520 (S17W75), although it appears that Region
1521 (S19W85) was involved in the early phase and may have been the
initial trigger for the overall event. An associated, bright CME was
observed off the southwest limb beginning at 1400Z; the leading edge
plane-of-sky speed was estimated to be about 960 km/s in the LASCO
C3 field of view. The proximity of Regions 1519 (S17 just past west
limb), 1520, and 1521 to the west limb hindered analysis of the spot
groups. New Region 1524 (S18E52) was assigned and is a simple C-type
sunspot group. An additional new spot group appeared to be emerging
just south of Region 1524.
IB. Previsione dell'Attività Solare
Solar activity is expected to be
moderate for the next 24 hours with 1520 and 1521 as the most likely
source regions. Activity and background levels are expected to
decrease significantly by the second and third days as these regions
rotate beyond west limb.
IIA. Sommario dell'Attività Geofisica dalle 2100Z-16 alle 2100Z-17
The geomagnetic field ranged from active to quiet levels with some
isolated minor and major storm intervals at high latitudes.
Unsettled to active levels prevailed duing the earlier part of the
period and quiet to unsettled levels dominated from 17/0900Z through
the end of the day. Solar wind observations from the ACE spacecraft
showed continued influence of the 12 July CME from the beginning of
the period through about 17/0600Z. The z-component of the
interplanetary magnetic field was initially negative and reached a
peak negative value of about -9 nT during this latter phase of the
CME passage. Nominal solar wind conditions prevailed from 17/0600Z
through the end of the day. A greater than 10 MeV proton event began
at 17/1715Z in response to todays long-duration M1 and associated
CME event. The peak value observed so far was 87 PFU at 17/2030Z.
The greater than 2 MeV electron flux at geosynchronous orbit reached
high levels during the period.
IIB. Previsione dell'Attività Geofisica
The geomagnetic field is
expected to be quiet for the next three days. Model results for
todays CME from the west limb indicate an interplanetary
disturbance that is too far west to produce geomagnetic activity.
The greater than 10 MeV proton event is expected to continue through
part of the first day (18 July).
III. Probabilità dell'Evento dalle Jul del 18 alle Jul del 20
Classe M | 55% | 40% | 25% |
Classe X | 10% | 10% | 05% |
Protone | 95% | 20% | 05% |
PCAF | yellow
|
IV. Flusso di 10.7 cm di Penticton
Osservato 17 Jul 128
Previsto 18 Jul-20 Jul 115/105/095
Media di 90 Giorni 17 Jul 129
V. Indici Geomagnetici A
Osservato Afr/Ap 16 Jul 027/040
Stimato Afr/Ap 17 Jul 015/020
Previsto Afr/Ap 18 Jul-20 Jul 006/005-007/005-006/005
VI. Probabilità dell'Attività Geomagnetica dal 18 Jul al 20 Jul
A. Latitudini Medie |
Attivo | 05% | 05% | 05% |
Tempesta minore | 01% | 01% | 01% |
Tempesta maggiore-grave | 01% | 01% | 01% |
B. Latitudini Alte |
Attivo | 15% | 15% | 15% |
Tempesta minore | 10% | 10% | 10% |
Tempesta maggiore-grave | 05% | 05% | 05% |
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