Publié: 2016 Apr 03 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 03 Apr 2016 | 080 | 014 |
| 04 Apr 2016 | 081 | 018 |
| 05 Apr 2016 | 082 | 018 |
Solar flaring activity was restricted to a single B2 event at the start of the period. NOAA 2526 remained quiet. No earth-directed coronal mass ejections (CMEs) were observed. The x-ray background flux was steady at the A7 level.
Quiet conditions are expected to continue.
The Kp index reached minor storming levels on 2 April during the 15-18UT interval, and moderate geomagnetic storming during the 21-24UT interval. K Dourbes was resp. at minor storming and active conditions. This geomagnetic activity was the result of the arrival of a co-rotating interaction region and associated wind stream from a negative coronal hole.
Solar wind speeds continued to gradually increase from about 330 km/s at 08:00UT to about 530 km/s around 21:30UT. A sharp drop in wind density from 40 to 7 particles per cm3 occurred at 14:05UT, coinciding with a final shift in the direction of the interplanetary magnetic field from away to towards the Sun. It was followed about an hour later by a strong dive of Bz towards negative values around -14 nT, with sustained but gradually weakening negative values over the subsequent 7 hours.
Currently, wind speed is declining with values near 400 km/s, and Bz varying between -5 and +5 nT. Mostly unsettled to active geomagnetic conditions are expected for the rest of the day (3 April), a minor storming episode not excluded. The wind stream from an elongated negative coronal hole between latitudes +10 and +30 degrees is still expected to influence the earth environment starting from 4 April onwards.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 013, sur la base de 18 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 082 |
| AK Chambon La Forêt | 041 |
| AK Wingst | 023 |
| Ap estimé | 019 |
| Nombre international de taches solaires estimé | 012 - Basé sur 20 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 | 25/02/2026 | M2.4 |
| Dernier orage géomagnétique | 22/02/2026 | Kp5+ (G1) |
| Jours sans taches solaires | |
|---|---|
| 365 derniers jours | 3 jours |
| 2026 | 3 jours (5%) |
| Dernier jour sans taches solaires | 24/02/2026 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| janvier 2026 | 112.6 -11.4 |
| mars 2026 | 85 -27.6 |
| 30 derniers jours | 71 -47.7 |