Affichage des archives de samedi, 26 mars 2011

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 2011 Mar 26 2200 UTC
Fait par le NOAA © SWPC et adapté par SpaceWeatherLive.com

Rapport de l'USAF/NOAA sur l'activité solaire et géophysique

SDF numéro 085 publié à 2200Z le 26 Mar 2011

IA. Analyse des régions solaires actives et activité du 25-2100Z au 26-2100Z

Solar activity was moderate due to an impulsive M1 X-ray event at 25/2322Z from Region 1176 (S16E16). Associated with this event were Type II (673 km/s), Type IV and 10.7 cm (170 sfu) radio signatures. Region 1176 remained mostly unchanged through the period, though it increased in longitudinal extent, and is classified as an F-type group. Region 1178 (S15E43) developed penumbra in its trailer spots to become a D-type group. At about 26/0500Z, GOES-15 SXI BE12A imagery observed a large surge from Region 1180 (N25E53) that appeared to continue for about six hours. X-ray data was mostly unavailable during this event due to GOES-13 and GOES-15 eclipse phase. Associated with this event was a fast-moving (approximately 850 km/s) partial-halo, asymmetric CME first observed in LASCO C3 imagery at 26/0630Z and STEREO-A and B COR2 imagery at 26/0709Z. Though this CME does not appear to have an Earth-directed component, further analysis is required.
IB. Prévisions d'activité solaire
Solar activity is expected to be low for the next three days (27 - 29 March). A chance for M-class activity exists on day one (27 March) becoming likely on days two and three (28 - 29 March) with a slight chance for X-class activity on 29 March. This expected increase in activity is due to the complex nature of Region 1176 and the return of old Region 1166 (N10, L=110) on 27 March. On its last transit across the disk, old Region 1166 produced four M-class events and one X-class event.
IIA. Résumé de l'activité géophysique du 25-2100Z au 26-2100Z
The geomagnetic field was at quiet levels. ACE solar wind data indicated a gradual decrease in wind velocities from a high of 460 km/s at 26/0243Z to a low of 360 km/s at 26/1841Z. IMF Bz was predominately north through the period.
IIB. Prévision de l'activité géophysique
The geomagnetic field is expected to be at mostly quiet levels for day one (27 March). By day two (28 March), quiet to unsettled conditions, with isolated active periods, are possible due to effects from the 24 March CME. Quiet levels are expected to return on day three (29 March).
III. Probabilité d'éruption solaire du 27 Mar au 29 Mar
Classe M50%60%70%
Classe X05%05%10%
Proton01%01%01%
PCAFgreen
IV. Flux Penticton 10.7 cm
  Observé       26 Mar 115
  Prévisionnel   27 Mar-29 Mar  120/125/125
  Moyenne des 90 derniers jours        26 Mar 096
V. Indice géomagnetique A
  Observé Afr/Ap 25 Mar  002/003
  Estimé     Afr/Ap 26 Mar  002/003
  Prévisionnel    Afr/Ap 27 Mar-29 Mar  005/005-010/010-005/005
VI. Probabilités d'activité géomagnétique du 27 Mar au 29 Mar
A. Latitudes moyennes
Actif10%20%10%
Tempête mineure01%05%01%
Tempête majeure/sévère01%01%01%
B. Hautes latitudes
Actif15%25%15%
Tempête mineure01%10%01%
Tempête majeure/sévère01%01%01%

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