Publié: 2016 Sep 18 1358 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 18 Sep 2016 | 080 | 015 |
| 19 Sep 2016 | 078 | 008 |
| 20 Sep 2016 | 077 | 007 |
Solar activity was low in the past 24 hours. Only one B4.1 flare was observed today (18-Sep-2016) from active region (AR 2592) which peaked at 02:51 UT. One additional active region is presently observed on the solar disk with the simple magnetic configuration. No Earth-directed CMEs were observed. There is a negative polarity coronal hole presently observed in the geoeffective position of the visible solar disk. Solar protons have remained at background levels over the past 24 hours. Solar activity is expected to be low with a small probability of C-class flares. The variations of the solar wind parameters slightly increased due to the influence of the negative polarity coronal hole currently observed on the visible side of the solar disk. Solar wind speed gradually increased from 310 to 370 km/s. The magnitude of the Interplanetary Magnetic Field (Bt) has increased from 5 to 7 nT, while Bz has fluctuated between +7 and -7 nT during last 24 hr being mainly negative. In the past 24 hours geomagnetic conditions have been quiet ( K Dourbes between 0 and 2; NOAA Kp between 0 and 2). However today at 12:00 UT both K Dourbes and Kp NOAA increased till 3 as the response to the solar wind parameters perturbations. Geomagnetic conditions are expected to be active over next 9-12 hours (Kp NOAA may increase till 4), then geomagnetic conditions are expected to return to mostly quiet levels over the next few days in view of the gradually waning effects of the coronal hole elevated speed stream.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 038, sur la base de 18 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 080 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 003 |
| Ap estimé | 003 |
| Nombre international de taches solaires estimé | 014 - Basé sur 25 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
De nombreuses personnes consultent SpaceWeatherLive pour suivre l'activité solaire ou observer les aurores boréales, mais l'augmentation du trafic engendre des coûts plus élevés pour maintenir les serveurs en ligne. Si vous appréciez SpaceWeatherLive et souhaitez soutenir le projet, vous pouvez vous abonner pour un site sans publicité ou faire un don. Grâce à votre aide, SpaceWeatherLive restera accessible !
| Dernière classe X | 04/02/2026 | X4.21 |
| Dernière classe M | 16/02/2026 | M2.4 |
| Dernier orage géomagnétique | 16/02/2026 | Kp6 (G2) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| janvier 2026 | 112.6 -11.4 |
| février 2026 | 106.5 -6.1 |
| 30 derniers jours | 123.7 +20 |