Affichage des archives de samedi, 15 juillet 2017

Bulletin quotidien sur l'activité solaire et géomagnétique du SIDC

Publié: 2017 Jul 15 1230 UTC

Prévisions SIDC

Valable à partir de 1230 UTC, 15 Jul 2017 jusqu'à 17 Jul 2017
Éruptions solaires

C-class flares expected, (probability >=50%)

Géomagnétisme

Active conditions expected (A>=20 or K=4)

Moniteur de Flux de Proton

Proton event expected (10 pfu at >10 MeV)

Flux de 10 cmAp
15 Jul 2017095003
16 Jul 2017097010
17 Jul 2017098014

Bulletin

NOAA AR 2665 produced four B and three C-class flares during the past 24 hours. The most intensive flare was C1.7-class flare peaking at 00:28 UT on 15-July. NOAA AR 2667 produced two radio bursts of type III. No Earth directed Coronal Mass Ejections (CMEs) have been detected. The integral proton flux for protons with energy above 10 meV (>10 MeV) at the geosynchronous orbit started to rise yesterday at 04:10 UT (14-July), it exceeded the solar radiation storm threshold of 10 pfu around 07:40 UT (14-July) and abruptly reached the peak of 22 pfu around 23:30 UT (14-July). Now (12:30 UT) the > 10 MeV integral proton flux decreased again till 13 pfu. More C-class flares are expected. The > 10 MeV proton flux is expected to go below the threshold level of 10 pfu (from 20:00 UT today). The arrival of 14-July HALO CME may rise again the values of the > 10 MeV proton flux up to 10 pfu (from midnight 16-July). Solar wind parameters were at low level. Small negative polarity southern coronal hole appeared not to be geoeffective. Total magnetic field remained below 4 nT, while Bz component was fluctuating between +/-2 nT over the past 24 hours. Solar wind speed gradually decreased from 370 km/s till 320 km/s. Small and abrupt change in solar wind parameters were observed yesterday at 16:20 UT. Those signatures may indicate a presence of a very small shock wave (as the possible reason of > 10 MeV integral proton flux additional acceleration). Geomagnetic conditions were very quiet. Planetary index Kp remained stable around Kp = 1, while the local K index (Dourbes) was fluctuating between 1 and 3. The geomagnetic field is expected to remain at the quiet level today, while from tomorrow (16 July late) minor storm can be expected (till Kp = 5) due to the 14-July-2017 Halo CME.

Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 034, sur la base de 18 stations.

Indices solaires pour 14 Jul 2017

Nombre de Wolf, observé par Catania052
Flux solaire à 10 cm094
AK Chambon La Forêt007
AK Wingst003
Ap estimé003
Nombre international de taches solaires estimé054 - Basé sur 37 stations

Résumé des événements marquants

JourCommencerMaxFinLocForceOP10cmCatania/NOAATypes de sursaut radio
Aucun

Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive

Toutes les heures sont indiquées en UTC

<< Aller à l'aperçu quotidien

Dernières nouvelles

Aidez SpaceWeatherLive.com !

A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!

No Ads on SWL Pro!
No Ads on SWL Pro! Abonnements
Donations
Aidez SpaceWeatherLive.com ! Faites un don
Soutenir SpaceWeatherLive avec nos produits dérivés
Découvrez nos produits dérivés

La Météo Spatiale en faits

Dernière classe X08/12/2025X1.1
Dernière classe M29/12/2025M1.0
Dernier orage géomagnétique22/12/2025Kp5 (G1)
Jours sans taches solaires
Dernier jour sans taches solaires08/06/2022
Nombre mensuel moyen de taches solaires
novembre 202591.8 -22.8
décembre 2025117.2 +25.4
30 derniers jours117.2 +28.6

A ce jour dans l'histoire*

Éruptions solaires
12023X5.01
22013M9.26
32011M3.51
42024M2.91
52024M2.75
DstG
11957-129G2
21967-109G2
32015-105G2
41989-100G2
51993-63G1
*depuis 1994

Les réseaux sociaux