Affichage des archives de samedi, 27 juillet 2002

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 2002 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 208 publié à 2200Z le 27 Jul 2002

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

Solar activity increased to high levels. Region 44 (S22E03) produced two major flares early in the period: an M8/2n at 26/2112 UTC and an M5 at 26/2217 UTC, both associated with moderate to strong discrete radio bursts. The M8 flare was also associated with a full-halo CME. Both major flares occurred along the magnetic neutral line separating Regions 44 and 39 (S16E07). Some decay was observed in the leader spots of Region 44, but it remained large and magnetically complex with a magnetic delta configuration evident within its intermediate spots. Region 39 produced isolated C-class flares including a C9/Sf at 27/0212 UTC. It also remained large and complex, but changed little during the period. Strong magnetic delta configurations persisted within its leading and trailing spots. Region 45 (N06W25) was in a growth phase and displayed minor polarity mixing. New Region 51 (S17E65) was assigned.
IB. Prévisions d'activité solaire
Solar activity is expected to be at moderate to high levels. Isolated M-class flares are expected from Regions 39 and 44. There is also a fair chance for a major flare from either of these regions.
IIA. Résumé de l'activité géophysique du 26-2100Z au 27-2100Z
Geomagnetic field activity was at unsettled to active levels during most of the period. This activity may have been due to a weak high-speed solar wind stream. The greater than 10 MeV proton event that began at 22/0655 UTC ended at 27/0320 UTC. The maximum flux for this event was 28 pfu at 23/1025 UTC.
IIB. Prévision de l'activité géophysique
Geomagnetic field activity is expected to be at unsettled levels at the start of the period. Activity is expected to increase to active to major storm levels beginning late on 28 July as today's halo CME reaches Earth. This disturbance is expected to subside to mostly unsettled levels by 30 July. There is a chance for a greater than 10 MeV proton event during the period.
III. Probabilité d'éruption solaire du 28 Jul au 30 Jul
Classe M80%80%80%
Classe X30%30%30%
Proton20%20%20%
PCAFyellow
IV. Flux Penticton 10.7 cm
  Observé       27 Jul 231
  Prévisionnel   28 Jul-30 Jul  230/225/220
  Moyenne des 90 derniers jours        27 Jul 164
V. Indice géomagnetique A
  Observé Afr/Ap 26 Jul  010/017
  Estimé     Afr/Ap 27 Jul  013/017
  Prévisionnel    Afr/Ap 28 Jul-30 Jul  010/012-025/030-018/020
VI. Probabilités d'activité géomagnétique du 28 Jul au 30 Jul
A. Latitudes moyennes
Actif30%40%30%
Tempête mineure10%20%10%
Tempête majeure/sévère01%10%05%
B. Hautes latitudes
Actif35%45%35%
Tempête mineure15%25%15%
Tempête majeure/sévère01%15%10%

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