Publié: 2019 Mar 06 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 06 Mar 2019 | 072 | 009 |
| 07 Mar 2019 | 072 | 010 |
| 08 Mar 2019 | 072 | 010 |
The solar activity has been quiet over the past 24 hours. The X-ray flux remains below B-level. From the two regions that showed some mild activity yesterday, one is now associated with a sunspot (Catania sunspot group 9, NOAA 2734) and produced small A-class flares. Solar activity is expected to remain at low levels with a small chance of C-class flare.
No Earth directed Coronal Mass Ejection has been observed. The greater than 10 MeV solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.
The solar wind parameters are currently slightly enhanced due to several small patchy equatorial coronal holes (negative polarity) located on the East hemisphere on Geo-effective area of the Sun. During the last 24-hour, the solar wind speed globally increased from about 350 km/h to 500 km/h, and the total interplanetary magnetic field strength also showed a slow increased from about 5 nT to 10 nT. The Bz component fluctuated between -8.5 nT and 8.5 nT. The solar wind parameters are expected to remain slightly enhanced due to those patchy equatorial coronal holes for the following days.
The geomagnetic conditions were quiet to unsettle over the past 24 hours, with K-index (Dourbes) ranging from 1 and 2, and Kp (NOAA) ranging from 1 and 3. In response to the slightly enhanced interplanetary magnetic field due to the small patchy equatorial coronal holes and possible prolonged period of southward directed Bz component, the geomagnetic conditions are expected to remain quiet to unsettle, short period of minor storm is possible but not likely.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 016, sur la base de 11 stations.
| Nombre de Wolf, observé par Catania | 027 |
| Flux solaire à 10 cm | 072 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 006 |
| Ap estimé | 004 |
| Nombre international de taches solaires estimé | 008 - Basé sur 32 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
A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!
| Dernière classe X | 08/12/2025 | X1.1 |
| Dernière classe M | 17/01/2026 | M2.2 |
| Dernier orage géomagnétique | 16/01/2026 | 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 |
| janvier 2026 | 96.7 -27.3 |
| 30 derniers jours | 101.3 -5.7 |