Affichage des archives de jeudi, 3 avril 2003
Rapport d'activité solaire
Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Rapport d'activité solaire et géophysique 2003 Apr 03 2200 UTC
Fait par le NOAA © SWPC et adapté par SpaceWeatherLive.comRapport de l'USAF/NOAA sur l'activité solaire et géophysique
SDF numéro 093 publié à 2200Z le 03 Apr 2003
IA. Analyse des régions solaires actives et activité du 02-2100Z au 03-2100Z
Solar activity has been at low levels. A significant
C-class flare from Region 324 (S11W35) occurred at 1027 UTC. This
region has rapidly increased in both size and complexity over the
last 24 hours. New Regions 329 (N01E18) and 330 (N07E74) were
numbered today. No other significant activity occurred.
IB. Prévisions d'activité solaire
Solar activity is expected to be
moderate. Regions 324 (S11W35) and 321 (N08W54) are sufficiently
complex and should continue to be for the next three days.
IIA. Résumé de l'activité géophysique du 02-2100Z au 03-2100Z
The geomagnetic field was at unsettled levels. The high speed stream
which began on 30 March is subsiding, but continued instability in
the interplanetary magnetic field is maintaining our unsettled
activity levels. The greater than 2 MeV electrons at geosynchronous
orbit reached high levels.
IIB. Prévision de l'activité géophysique
The geomagnetic field is
expected to be at quiet to unsettled levels with isolated periods of
active for the next two days due to the subsiding high speed stream.
By day three, the solar wind will increase again, and combined with
the potential for southward Bz, is likely to cause an increase to
unsettled to active levels with isolated periods of minor storming.
III. Probabilité d'éruption solaire du 04 Apr au 06 Apr
Classe M | 45% | 45% | 35% |
Classe X | 10% | 10% | 05% |
Proton | 10% | 10% | 05% |
PCAF | green
|
IV. Flux Penticton 10.7 cm
Observé 03 Apr 156
Prévisionnel 04 Apr-06 Apr 155/155/150
Moyenne des 90 derniers jours 03 Apr 135
V. Indice géomagnetique A
Observé Afr/Ap 02 Apr 011/020
Estimé Afr/Ap 03 Apr 015/013
Prévisionnel Afr/Ap 04 Apr-06 Apr 010/010-010/012-008/012
VI. Probabilités d'activité géomagnétique du 04 Apr au 06 Apr
A. Latitudes moyennes |
Actif | 25% | 25% | 25% |
Tempête mineure | 10% | 10% | 10% |
Tempête majeure/sévère | 05% | 05% | 05% |
B. Hautes latitudes |
Actif | 40% | 40% | 40% |
Tempête mineure | 15% | 20% | 20% |
Tempête majeure/sévère | 05% | 05% | 05% |
VII. Comments: Beginning 1500 UTC April 8, SEC will begin using data from the GOES 12 satellite, and stop receiving GOES 8 data. GOES 12 has the new Solar X-Ray Imager (SXI), which will acquire real-time, operational images of the solar x-ray flux. With the switch from GOES 8 to GOES 12, the primary/secondary designations will change. GOES 12 will be the primary satellite for the SXI. All other data, including magnetometer, XRS x-ray measurements, and energetic particles, will have GOES 10 as their primary source, with GOES 12 as the secondary source where available. Please see http://www.sec.noaa.gov/GOES.html for important information on this changeover.
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