Publié: 2020 Apr 30 1234 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 30 Apr 2020 | 070 | 003 |
| 01 May 2020 | 070 | 009 |
| 02 May 2020 | 071 | 015 |
Solar X-ray flux remained below B level. Active Region (AR) 2760 showed some further sunspot emergence, while newly numbered region AR 2762 showed signs of decay. The AR 2761 is now only a plage region. Solar flaring activity is expected to remain at very low levels.
No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery in the last 24 hours.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to stay at nominal levels for the next 24 hours. The greater than 2 MeV electron flux was between nominal and moderate levels over the past 24 hours and is expected to be at nominal to moderate levels over the next 24 hours.
The solar wind speed near Earth decreased from around 370 km/s to 270 km/s and the total magnetic field varied between 2 and 4 nT (DSCOVR) over the past 24 hours. The Interplanetary Magnetic Field (IMF) was predominantly oriented towards the Sun (phi angle in the negative sector. Bz was mostly negative, with a minimum value of around -3 nT. Nominal solar wind conditions are expected for Apr 30 - May 01. The filament eruption observed on April 27 that possibly had an Earth directed component may produce a slight enhancement in solar wind parameters at Earth on May 02.
Geomagnetic conditions were quiet (local K Dourbes and NOAA Kp recorded values between 0-2 and 0-1, respectively). Quiet geomagnetic conditions are expected for Apr 30 - May 01 with isolated unsettled episodes possible. The possibility of an active interval on May 02, due to a possible interaction with the eruption of Apr 27, is also not excluded.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 020, sur la base de 28 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 070 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 004 |
| Ap estimé | 003 |
| Nombre international de taches solaires estimé | 023 - Basé sur 23 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 |
| 30 derniers jours | 72.7 -45.8 |