Publié: 2017 Jan 27 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 27 Jan 2017 | 082 | 022 |
| 28 Jan 2017 | 081 | 017 |
| 29 Jan 2017 | 080 | 007 |
Solar activity was very low. B-class flare production by NOAA 2629 pretty much stalled. NOAA 2627, now spotless, produced the strongest event of the period: an isolated B5 flare peaking at 10:45UT. NOAA 2628 showed some filament activity in its middle portion around midnight. No earth- directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10MeV proton flux was at nominal levels.
Mostly quiet flaring conditions are expected, with a small chance on a C-class event.
Around 26/13:45UT January, solar wind speed gradually increased from an initial 375 km/s up to values near 670 km/s around 06UT on 27 January. This is the High Speed Stream (HSS) from the positive equatorial coronal hole (CH), arriving somewhat earlier than expected. It was preceded by a co- rotating interaction region (CIR) that drove a weak shock on 26/07:12UT January. Bz oscillated wildly between -12 nT and +13 nT, preventing the development of a geomagnetic storm. Since 06UT, Bz varied between +5 nT and -5 nT, and wind speed at 560 km/s. The interplanetary magnetic field was mostly directed away from the Sun.
The geomagnetic field was at quiet to active levels. The earth environment will probably remain under the influence of the HSS until at least 28 January. Quiet to active geomagnetic conditions are expected, with a minor storming episode not excluded.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 027, sur la base de 16 stations.
| Nombre de Wolf, observé par Catania | 053 |
| Flux solaire à 10 cm | 083 |
| AK Chambon La Forêt | 035 |
| AK Wingst | 012 |
| Ap estimé | 015 |
| Nombre international de taches solaires estimé | 041 - Basé sur 31 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 | 03/02/2026 | X1.5 |
| Dernière classe M | 03/02/2026 | M3.4 |
| Dernier orage géomagnétique | 28/01/2026 | Kp5+ (G1) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| décembre 2025 | 124 +32.2 |
| février 2026 | 133 +9 |
| 30 derniers jours | 120.6 +10.9 |