Publié: 2021 Jul 26 1238 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 26 Jul 2021 | 080 | 006 |
| 27 Jul 2021 | 080 | 014 |
| 28 Jul 2021 | 080 | 012 |
The solar activity has been quiet over the past 24 hours, with the X-ray flux below C-level. Two sunspot groups are currently visible on the solar disc (Catania sunspot group 22 / NOAA AR-2846, and Catania sunspot group 23 / NOAA AR-2847). They have not produced any significant flare. The solar activity is expected to remain mostly low levels over the next 24 hours with possible C-class flare.
No Earth directed Coronal Mass Ejection (CME) has been detected in the available coronagraph imagery.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux was below the 1000 pfu threshold in the past 24 hours and is expected to remain so during the next 24 hours. The 24h electron fluence was at normal levels in the last 24 hours and is expected to stay at normal levels for the next 24 hours.
The solar wind parameters (as observed by ACE and DSCOVR) show an ambient background and slow solar wind speed regime. The solar wind speed ranged from 301 km/s to 446 km/s. The interplanetary magnetic field magnitude was below 5.0 nT, and Bz components varied between -4.0 nT and 3.9 nT. The high-speed streams associated with the mid-latitude extension of the positive polarity northern polar Coronal Hole, reported crossing the central meridian on July 24th is expected to enhance the solar wind condition on July 27 and persist for several days.
The geomagnetic conditions were mostly quiet over the past 24 hours. The conditions are expected to remain mostly quiet as the Earth is expected to remain in slow solar wind speed regime for the next 24 hours. Then, the conditions are expected to be unsettled to active with the arrival of the high-speed streams associated with northern polar Coronal Hole in July 27-28.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 032, sur la base de 19 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 082 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 003 |
| Ap estimé | 002 |
| Nombre international de taches solaires estimé | 031 - 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 | 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 |