Affichage des archives de dimanche, 30 septembre 2001

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 2001 Sep 30 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 273 publié à 2200Z le 30 Sep 2001

IA. Analyse des régions solaires actives et activité du 29-2100Z au 30-2100Z

Solar activity remained at moderate levels. Region 9628 (S17W76) produced a long-duration M1/Sf flare at 30/1141 UTC associated with minor discrete frequency radio emission. Region 9628 may have decayed a bit as it approached the west limb, but remained large and complex. Decay was also noted in Region 9632 (S18W61) as its large interior spot mass began to split, which may have dissipated the magnetic delta structure contained therein. Nonetheless, this region remained large and complex. Region 9636 (N14W15), a reverse-polarity sunspot group, showed gradual development during the day. It was moderate in size and complexity as it produced isolated subflares, none of which were associated with significant X-ray or radio emission.
IB. Prévisions d'activité solaire
Solar activity is expected to remain at moderate levels. Isolated M-class flares will be possible from Regions 9628, 9632, and 9636. Regions 9628 and 9632 each could produce an isolated major flare before they rotate out of view on 01 and 02 October, respectively.
IIA. Résumé de l'activité géophysique du 29-2100Z au 30-2100Z
Geomagnetic field activity ranged from quiet to minor storm levels. Minor storm levels occurred globally during 29/2100 - 2400 UTC following a sustained period of southward IMF Bz (as measured by NASA's ACE spacecraft). Activity decreased to quiet to unsettled levels during 30/0000 - 1500 UTC, then increased to active levels for the rest of the period. An interplanetary shock passed the ACE spacecraft at 30/1848 UTC. The source for this shock may have been a CME that followed a long-duration M3/2n flare from Region 9636 at 28/0830 UTC. The greater than 10 MeV event that began at 24/1215 UTC ended at 30/1710 UTC.
IIB. Prévision de l'activité géophysique
Active geomagnetic conditions will be possible during 01 - 02 October due to recent CME activity. Field activity is expected to decrease to quiet to unsettled levels on 03 October. There will be a slight chance for a proton flare from Region 9628 or 9632 during the period.
III. Probabilité d'éruption solaire du 01 Oct au 03 Oct
Classe M80%75%70%
Classe X25%20%10%
Proton20%15%10%
PCAFyellow
IV. Flux Penticton 10.7 cm
  Observé       30 Sep 236
  Prévisionnel   01 Oct-03 Oct  230/225/225
  Moyenne des 90 derniers jours        30 Sep 176
V. Indice géomagnetique A
  Observé Afr/Ap 29 Sep  019/021
  Estimé     Afr/Ap 30 Sep  012/012
  Prévisionnel    Afr/Ap 01 Oct-03 Oct  020/015-015/012-012/012
VI. Probabilités d'activité géomagnétique du 01 Oct au 03 Oct
A. Latitudes moyennes
Actif40%40%30%
Tempête mineure20%20%10%
Tempête majeure/sévère10%10%01%
B. Hautes latitudes
Actif50%50%35%
Tempête mineure25%25%15%
Tempête majeure/sévère15%15%01%

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