Affichage des archives de mardi, 27 juillet 2004

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 2004 Jul 27 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 209 publié à 2200Z le 27 Jul 2004

IA. Analyse des régions solaires actives et activité du 26-2100Z au 27-2100Z

Solar activity was moderate. Region 652 (N07W62) produced three M1 flares this period. Region 652 continues to slowly decay as it approaches the west limb. It still maintains considerable size and a complex delta configuration. No other significant changes were observed on the disk or limb.
IB. Prévisions d'activité solaire
Solar activity is expected to be moderate. Continued M-class activity is expected from Region 652 and there is a slight chance for a major flare.
IIA. Résumé de l'activité géophysique du 26-2100Z au 27-2100Z
The geomagnetic field ranged from unsettled to severe storming. A strong sudden impulse (SI) of 95 Nt was observed on the Boulder magnetometer at 26/2228Z. This SI followed the very fast (~31 hours) transit of the full halo CME associated with the long duration M1 flare on 25/1514Z. Solar wind speed increased from the already elevated levels near 600 km/s to over 1050 km/s. After approximately four hours of fluctuating between -15 and +15 nT, the IMF Bz rotated strong southward and ranged from -15 to -25 nT for about 15 hours. The fast solar wind speed and southward Bz combined to produce severe geomagnetic storm levels at all latitudes from 27/0000Z to 27/1500Z. Solar wind speed was still near 800 km/s by the end of the period and the disturbance had declined to minor storm levels. The greater than 10 MeV proton event that began on 25/1855Z is still in progress. A rapid, short-lived increase in the greater than 10 MeV protons to 2,090 pfu occurred with the shock passage. Protons quickly declined and were straddling the 10 pfu alert threshold by the end of the period. The greater than 2 MeV electrons at geosynchronous orbit were at high levels.
IIB. Prévision de l'activité géophysique
The geomagnetic field is expected to range from quiet to major storm levels. The most disturbed periods are expected during the first half of day one as the current major disturbance subsides. Mostly quiet to unsettled conditions are expected on 29 - 30 July.
III. Probabilité d'éruption solaire du 28 Jul au 30 Jul
Classe M55%40%10%
Classe X10%05%05%
Proton99%10%05%
PCAFyellow
IV. Flux Penticton 10.7 cm
  Observé       27 Jul 118
  Prévisionnel   28 Jul-30 Jul  110/105/090
  Moyenne des 90 derniers jours        27 Jul 106
V. Indice géomagnetique A
  Observé Afr/Ap 26 Jul  026/031
  Estimé     Afr/Ap 27 Jul  120/180
  Prévisionnel    Afr/Ap 28 Jul-30 Jul  020/025-010/015-008/010
VI. Probabilités d'activité géomagnétique du 28 Jul au 30 Jul
A. Latitudes moyennes
Actif50%35%20%
Tempête mineure25%05%05%
Tempête majeure/sévère15%01%01%
B. Hautes latitudes
Actif50%40%20%
Tempête mineure30%10%05%
Tempête majeure/sévère20%05%01%

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