Publié: 2014 Jul 10 1255 UTC
Active (M-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 10 Jul 2014 | 200 | 012 |
| 11 Jul 2014 | 198 | 007 |
| 12 Jul 2014 | 198 | 011 |
Solar flare activity was limited to two C-class flares, originating from Catania sunspot regions 3 and 5 (NOAA AR 2104 and 2106 respectively), both located near the West limb. Catania region 16 (NOAA AR 2113) was stable and did not produce additional flares and also Catania sunspot regions 6 and 9 (NOAA 2108 and 2109 respectively) did not show much activity. Two partial halo CMEs were observed in coronagraphic imagery. The first CME (first measurement in SOHO/LASCO C2 at 16:36 UT on July 9) was associated with a filament eruption occurring near S00E15 and is propagating east from the Sun-Earth line with a projected plane of the sky speed of 520 km/s (CACTus estimation). The second CME (first measurement in SOHO/LASCO C2 at 7:12 UT on July 10) was associated with a prominence eruption occurring near Catania region 3 and is propagating west from the Sun-Earth line with a projected plane of the sky speed of 760 km/s (CACTus estimation). For the first CME, the arrival of a glancing blow from the CME-driven shock wave is expected on July 13 near 0 UT. The second CME has less chances to arrive at Earth, but minor signatures of arrival might still be possible on the UT morning of July 13. Flaring activity is expected to continue with C-class flares and possibly an isolated M-class flare. Solar wind speed gradually increased from 350 to 400 km/s, as measured by ACE. The magnitude of interplanetary magnetic field was stable with values between 4 and 8 nT with a mainly negative Bz component. Geomagnetic conditions have been quiet to unsettled and are expected to remain so. At the possible arrival of a glancing blow July 8 CME, active conditions are expected from the evening of July 11.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 122, sur la base de 11 stations.
| Nombre de Wolf, observé par Catania | 184 |
| Flux solaire à 10 cm | 198 |
| AK Chambon La Forêt | 018 |
| AK Wingst | 010 |
| Ap estimé | 010 |
| Nombre international de taches solaires estimé | 127 - Basé sur 12 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio | |
|---|---|---|---|---|---|---|---|---|---|---|
| Aucun | ||||||||||
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
Toutes les heures sont indiquées en UTC
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!
| Dernière classe X | 18/01/2026 | X1.9 |
| Dernière classe M | 21/01/2026 | M3.4 |
| Dernier orage géomagnétique | 21/01/2026 | Kp7+ (G3) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| décembre 2025 | 124 +32.2 |
| janvier 2026 | 110 -14 |
| 30 derniers jours | 114.8 +6.7 |