Affichage des archives de jeudi, 5 avril 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 Apr 05 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 095 publié à 2200Z le 05 Apr 2001

IA. Analyse des régions solaires actives et activité du 04-2100Z au 05-2100Z

Solar activity was high. Two major flares were observed during the past 24 hours. The first was a long-duration M8 that peaked at 0922Z, originating from Region 9393 behind the west limb. This flare was associated with a CME which gives every indication of moving in a westward direction, perpendicular to the Earth-Sun line. The second was an M5/2n at 1725Z from Region 9415 (S21E47). This event had an extended maximum and a slow decay profile. An associated CME was just entering the C2 field of view at forecast issue time and did not appear to have any earthward component. Region 9415 appears to have formed a delta configuration in the leader portion of the group. Region 9417 (S08E27) grew rapidly during the last 24 hours and produced an M1/Sn flare at 0834Z. Today's 10.7 cm background flux of 210 SFU had to be estimated due to greatly enhanced radio noise levels occurring with today's long-duration flare activity.
IB. Prévisions d'activité solaire
Solar activity is expected to be mostly moderate during the next three days. There is a fair chance, however, for additional major flares from Region 9415.
IIA. Résumé de l'activité géophysique du 04-2100Z au 05-2100Z
The geomagnetic field was predominantly quiet to active during the past 24 hours. The first nine hours of the period were quiet, but activity increased to mostly active from 0600-2100Z. There was a minor storm period at high latitudes from 0900-1200Z. The greater than 10 MeV proton event continues in progress with a continued slow decline in flux levels. The flux at 05/2100Z was 25 pfu.
IIB. Prévision de l'activité géophysique
The geomagnetic field is expected to be mostly unsettled tomorrow, with a chance for some isolated active periods. Predominantly unsettled levels should prevail for the second and third days.
III. Probabilité d'éruption solaire du 06 Apr au 08 Apr
Classe M75%75%75%
Classe X20%20%20%
Proton99%20%20%
PCAFin progress
IV. Flux Penticton 10.7 cm
  Observé       05 Apr 210
  Prévisionnel   06 Apr-08 Apr  210/210/205
  Moyenne des 90 derniers jours        05 Apr 167
V. Indice géomagnetique A
  Observé Afr/Ap 04 Apr  012/015
  Estimé     Afr/Ap 05 Apr  015/015
  Prévisionnel    Afr/Ap 06 Apr-08 Apr  015/015-012/008-012/008
VI. Probabilités d'activité géomagnétique du 06 Apr au 08 Apr
A. Latitudes moyennes
Actif30%25%20%
Tempête mineure15%10%10%
Tempête majeure/sévère10%05%05%
B. Hautes latitudes
Actif30%25%20%
Tempête mineure20%15%10%
Tempête majeure/sévère15%10%10%

<< 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 M23/04/2024M2.9
Dernier orage géomagnétique19/04/2024Kp7 (G3)
Jours sans taches solaires
Dernier jour sans taches solaires08/06/2022
Nombre mensuel moyen de taches solaires
mars 2024104.9 -19.8
Last 30 days125.4 +21.1

A ce jour dans l'histoire*

Éruptions solaires
11998X1.77
22003M7.4
32001M5.77
42024M3.5
52024M3.0
ApG
1202365G4
2200227G2
3201226G2
4201736G1
5200827G1
*depuis 1994

Les réseaux sociaux