Affichage des archives de jeudi, 16 août 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 Aug 16 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 228 publié à 2200Z le 16 Aug 2001

IA. Analyse des régions solaires actives et activité du 15-2100Z au 16-2100Z

Solar activity from numbered regions on the visible disk was low. Impulsive B- and C-class flares were observed throughout the period, the largest being an optically uncorrelated C3 flare at 16/0957 UTC. However, the most impressive activity of the day was a remarkable backside CME, observed on SOHO/LASCO starting at about 15/2355 UTC. This event resulted in the proton enhancements discussed in section IIA below. The observed CME together with backside imagery inferred from the SOHO/MDI instrument suggest old Region 9557 (S20, L=283) as the likely source, presently located near the far backside central meridian. On the visible disk, three new regions were numbered today: 9583 (S23E13), 9584 (S11E60), and 9585 (N15E74). All appear to be small, simply structured beta-class groups with low flare activity potential.
IB. Prévisions d'activité solaire
Solar activity on the visible disk is expected to persist at mainly low levels for the next three days.
IIA. Résumé de l'activité géophysique du 15-2100Z au 16-2100Z
Geomagnetic field activity has been quiet to unsettled throughout the period. A major proton event for >= 100MeV protons above 1pfu began at 16/0105 UTC, followed by >= 10Mev protons above 10pfu at 16/0135 UTC. Maximum flux for 100Mev protons was 29pfu at 16/0305 UTC, and for 10MeV protons was 493pfu at 16/0355 UTC. Both events remain in progress, and represent a record response for a presumed CME source so far behind the western limb as described in section 1A above. Greater than 2MeV electrons were observed at moderate enhancement levels again today, although the electron sensor on GOES-8 was saturated by the proton event for much of the period.
IIB. Prévision de l'activité géophysique
The geomagnetic field is expected to be at active to minor storm levels within 24 hours, in response to anticipated shock passage from CME activity reported on August 14th. Isolated major storm periods may also be possible at higher latitudes, as well as an enhancement of 10MeV proton levels for the event in progress. Geomagnetic storm activity is expected to wane during day two, along with the 100MeV proton event. The 10MeV proton event is expected to persist at levels above 10pfu into day three. Greater than 2MeV electrons are also expected to persist at moderate enhancement levels.
III. Probabilité d'éruption solaire du 17 Aug au 19 Aug
Classe M25%25%25%
Classe X01%01%01%
Proton99%95%90%
PCAFred
IV. Flux Penticton 10.7 cm
  Observé       16 Aug 143
  Prévisionnel   17 Aug-19 Aug  140/140/145
  Moyenne des 90 derniers jours        16 Aug 151
V. Indice géomagnetique A
  Observé Afr/Ap 15 Aug  004/009
  Estimé     Afr/Ap 16 Aug  007/008
  Prévisionnel    Afr/Ap 17 Aug-19 Aug  025/020-017/015-012/018
VI. Probabilités d'activité géomagnétique du 17 Aug au 19 Aug
A. Latitudes moyennes
Actif35%30%25%
Tempête mineure20%15%10%
Tempête majeure/sévère10%05%05%
B. Hautes latitudes
Actif40%30%30%
Tempête mineure20%15%15%
Tempête majeure/sévère05%05%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 M27/04/2024M2.1
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 days138.1 +30.7

A ce jour dans l'histoire*

Éruptions solaires
11998X1.54
22006X1.13
32003M2.46
42024M2.1
52001M1.81
ApG
11956172G4
2195554G4
3193761G3
4196031G3
5199530G2
*depuis 1994

Les réseaux sociaux