Affichage des archives de jeudi, 28 juillet 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 Jul 28 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 209 publié à 2200Z le 28 Jul 2005

IA. Analyse des régions solaires actives et activité du 27-2100Z au 28-2100Z

Solar activity was moderate due to an M1 x-ray event at 0030 UTC from newly numbered Region 792 (N12E78). The event was associated with a CME off the east limb with a plane of sky speed of about 850 km/s. Region 792 is clearly the return of old Region 786, and is likely to have been the source of the recent series of CME's originating behind the east limb. The region was also responsible for the remainder of today's occasional C-class and B-class activity. Region 791 (N14W20), the only other spotted group on the Sun, was quiet and stable.
IB. Prévisions d'activité solaire
Solar activity is expected to moderate with Region 792 as the dominant source of activity. There is also a slight chance for major flare activity from this group.
IIA. Résumé de l'activité géophysique du 27-2100Z au 28-2100Z
The geomagnetic field was mostly unsettled to active with a minor storm period from 0300-0600 UTC. Solar wind data indicate the onset of a co-rotating interaction region late on the 27th followed by the onset of coronal hole stream by about midday on the 28th. Solar wind speed is currently steady at around 600 km/s. A greater than 10 MeV proton event began at 2300 UTC on the 27th and reached a maximum so far of 32 PFU at 1300 UTC on the 28th. The event continues in progress with a flux of 27 PFU at the end of the analysis interval. The main source for this event appears the shock driven by the fast CME of 27/0454 UTC. It should be noted, however, the flux levels were already enhanced prior to this event. This initial enhancement may have been caused by one or more of the earlier CME's that originated behind the east limb; for example the CME's of 26/0930 UTC, 25/1106 UTC, and 24/1418 UTC.
IIB. Prévision de l'activité géophysique
The geomagnetic field is expected to be mostly unsettled with a chance for some active periods for 29 July. Conditions are expected to decline to predominantly unsettled for 30 July and should be quiet to unsettled for 31 July. The greater than 10 MeV proton event is expected to end sometime on 29 July, provided that no new particles are accelerated by new activity from Region 792.
III. Probabilité d'éruption solaire du 29 Jul au 31 Jul
Classe M70%70%70%
Classe X10%10%10%
Proton90%10%10%
PCAFYellow
IV. Flux Penticton 10.7 cm
  Observé       28 Jul 096
  Prévisionnel   29 Jul-31 Jul  105/110/115
  Moyenne des 90 derniers jours        28 Jul 096
V. Indice géomagnetique A
  Observé Afr/Ap 27 Jul  015/017
  Estimé     Afr/Ap 28 Jul  016/030
  Prévisionnel    Afr/Ap 29 Jul-31 Jul  010/015-010/012-007/010
VI. Probabilités d'activité géomagnétique du 29 Jul au 31 Jul
A. Latitudes moyennes
Actif35%30%25%
Tempête mineure20%20%15%
Tempête majeure/sévère05%05%05%
B. Hautes latitudes
Actif30%30%25%
Tempête mineure25%25%15%
Tempête majeure/sévère10%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 X28/03/2024X1.1
Dernière classe M29/04/2024M3.6
Dernier orage géomagnétique26/04/2024Kp5+ (G1)
Jours sans taches solaires
Dernier jour sans taches solaires08/06/2022
Nombre mensuel moyen de taches solaires
mars 2024104.9 -19.8
Last 30 days139 +32.6

A ce jour dans l'histoire*

Éruptions solaires
11998M9.27
22024M3.6
32024M2.5
41999M1.7
52003M1.69
ApG
1195658G4
2195287G3
3199159G3
4196055G2
5197359G2
*depuis 1994

Les réseaux sociaux