Affichage des archives de jeudi, 8 septembre 2005

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 2005 Sep 08 2204 UTC
Fait par le NOAA © SWPC et adapté par SpaceWeatherLive.com

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

SDF numéro 251 publié à 2200Z le 08 Sep 2005

IA. Analyse des régions solaires actives et activité du 07-2100Z au 08-2100Z

Solar activity remains at high levels. An X5/2b flare was in progress from Region 808 (S09E67) at the time of this writing. Moderate centimetric radio bursts are also in progress, including a 990 sfu Tenflare. Very active Region 808 is rotating into view as a large and complex sunspot cluster. Limb proximity is still hindering the analysis, but this compact spot group will likely exceed 1000 millionths of white light area. Numerous C-class flares and two M2 flares preceded the X5 event. New Region 809 (N10E60) was numbered today.
IB. Prévisions d'activité solaire
Solar activity is expected to remain at high levels. Region 808 is a large and complex sunspot group capable of producing M and X-class flares.
IIA. Résumé de l'activité géophysique du 07-2100Z au 08-2100Z
The geomagnetic field was quiet to unsettled. A sudden disturbance of 41 nT (magnetic crochet) was observed in the geomagnetic field following today's X5 flare. A greater than 10 and greater than 100 MeV proton event occurred following yesterday's X17 flare on the southeast limb. The greater than 10 MeV proton event began at 08/0215Z and remains in progress. The peak flux so far was 87 pfu at 08/1950Z. The greater than 100 MeV proton event began at 08/0405Z and also remains in progress. The peak flux was 7 pfu at 08/1925Z. A greater than 100 MeV proton event from a source on the east limb is extremely rare. The greater than 2 MeV electron flux at geosynchronous orbit was at high levels again today.
IIB. Prévision de l'activité géophysique
The geomagnetic field is expected to range from quiet to minor storm levels. The CME associated with yesterday's X17 flare was very large and very fast. Although the magnetic cloud associated with this CME is not expected to impact Earth, a shock passage is expected, which will likely produce active to minor storm periods on 09 Sep. Isolated active periods are expected on 10 and 11 Sep. The greater than 10 MeV proton event currently in progress is expected to continue through 10 Sep. A further enhancement in the greater than 10 MeV protons will likely follow the anticipated shock passage on 09 Sep. Today's X5 flare may enhance the existing proton event. The greater than 100 MeV proton event will persist through 09 Sep.
III. Probabilité d'éruption solaire du 09 Sep au 11 Sep
Classe M80%80%80%
Classe X50%50%50%
Proton99%90%75%
PCAFin progress
IV. Flux Penticton 10.7 cm
  Observé       08 Sep 094
  Prévisionnel   09 Sep-11 Sep  100/110/110
  Moyenne des 90 derniers jours        08 Sep 091
V. Indice géomagnetique A
  Observé Afr/Ap 07 Sep  018/015
  Estimé     Afr/Ap 08 Sep  008/012
  Prévisionnel    Afr/Ap 09 Sep-11 Sep  020/025-015/020-008/010
VI. Probabilités d'activité géomagnétique du 09 Sep au 11 Sep
A. Latitudes moyennes
Actif40%30%25%
Tempête mineure20%15%10%
Tempête majeure/sévère10%05%01%
B. Hautes latitudes
Actif50%40%30%
Tempête mineure30%20%15%
Tempête majeure/sévère15%10%05%

<< Aller à l'aperçu quotidien

Dernières nouvelles

Aidez SpaceWeatherLive.com !

Vous êtes de plus en plus nombreux à consulter SpaceWeatherLive pour suivre l'activité solaire ou aurorale, et avec le traffic les coûts du serveur augmentent. Si vous appréciez SpaceWeatherLive, soutenez notre projet en faisant un don afin que nous puissions continuer à vous informer !

54%
Soutenir SpaceWeatherLive avec nos produits dérivés
Découvrez nos produits dérivés

La Météo Spatiale en faits

Dernière classe X03/05/2024X1.6
Dernière classe M03/05/2024M4.4
Dernier orage géomagnétique02/05/2024Kp7- (G3)
Jours sans taches solaires
Dernier jour sans taches solaires08/06/2022
Nombre mensuel moyen de taches solaires
avril 2024136.5 +31.6
Last 30 days149.4 +51.8

A ce jour dans l'histoire*

Éruptions solaires
12024X1.6
22022X1.1
32013M8.19
42023M7.2
51999M6.41
ApG
1197697G4
2198640G3
3196787G3
4197883G3
5195256G3
*depuis 1994

Les réseaux sociaux